corso di fisica nucleare - paolo finelli dip. fisica ed astronomia
Transcript
corso di fisica nucleare - paolo finelli dip. fisica ed astronomia
Physics of nuclear bombs CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 1 Physics of nuclear bombs A nuclear explosion is achieved by the rapid assembly, in a suitable geometry, of NEM with sufficient nuclear reactivity to initiate and sustain a chain reaction driven by fast neutrons. For this to happen, on average at least one of the several energetic neutrons released per fission in the NEM must be “productively” captured, i.e., it must produce another fission following its capture. The neutron must be productively captured before it is unproductively captured, loses too much energy, or escapes from the configuration. Dependence on the Concentration of the Fissile Material In order to produce an explosion, the fast neutrons from each fission must produce more fast neutrons in each successive “generation”, i.e., the neutron multiplication factor k must be > 1. Such a configuration is said to be “prompt supercritical”. Any mixture of nuclear-explosive nuclides and other nuclides that can support a fast-neutron chain reaction when present in suitable quantity, purity, and geometry is called nuclear-explosive material (NEM). CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 2 Tamper - neutron reflector • A reflector surrounding a configuration of fissile material will reduce the number of neutrons that escape through its surface. The best neutron reflectors are light nuclei that have have no propensity to capture neutrons. The lightest practical material is Beryllium, the lightest strong metal • In a nuclear weapon the envelope has an additional role: its very inertia delays the expansion of the reacting materia. The weapon tends to fly to bits as the reaction proceeds and this tends to stop the reaction, so the use of a tamper makes for a longer lasting, more energetic, and more efficient explosion. The most effective tamper is the one having the highest density (U238) CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 3 Physics of nuclear bombs The yield of a nuclear weapon is defined (roughly) as the total energy it releases when it explodes The energy release is quoted in units of the energy released by a ton of TNT 1 Kiloton (Kt) = 1 thousand tons of TNT 1 Megaton (Mt) = 1 million tons of TNT For this purpose the energy of 1 kt of TNT is defined as 1012 Calories = 4.2 x 1012 Joules Fission weapons • Theoretical maximum yield-to-weight ratio: 8,000 tons = 8 kt TNT from 1 lb. of NEM (~ 10,000,000 times as much per lb. as TNT) • Difficult to make weapons larger than few 100 kt (Yields of tested weapons: 1–500 kt) CORSO DI FISICA NUCLEARE - PAOLO FINELLI Thermonuclear weapons • Theoretical maximum yield-to-weight ratio: 25 kt TNT from 1 lb. of fusion material (~ 3 times as much per lb. as fission weapons) • But there is no fundamental limit to the size of a thermonuclear weapon DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 4 5 Gun design CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 6 © unmakingthebomb.com, blog.nuclearsecrecy.com CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 7 © unmakingthebomb.com, blog.nuclearsecrecy.com CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 8 © unmakingthebomb.com, blog.nuclearsecrecy.com CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 9 © unmakingthebomb.com, blog.nuclearsecrecy.com CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 10 © unmakingthebomb.com, blog.nuclearsecrecy.com CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 11 © unmakingthebomb.com, blog.nuclearsecrecy.com CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 12 © unmakingthebomb.com, blog.nuclearsecrecy.com CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 13 © unmakingthebomb.com, blog.nuclearsecrecy.com CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 14 © unmakingthebomb.com, blog.nuclearsecrecy.com CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA Gun design - Little boy CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 15 16 Plutonium Plutonium is rather brittle at room temperature, and is difficult to form into desired shapes unless alloyed with another metal. But common light alloying metals such as aluminum cannot be used because of the (a, n) problem; one has to use something heavier. Los Alamos metallurgists found that by alloying plutonium with 3 % gallium by weight, they could avoid the (a, n) problem while also depressing the melting point of the malleable δ-phase of plutonium sufficiently that it could be worked at room temperature. An advantage of this approach was that since the lower-density δ-phase transforms to the higherdensity α-phase under compression, one realizes a gain in the sense that the critical mass of α-phase plutonium is less than that of the δ-phase material that one began with, leading to an efficiency enhancement, significantly helping to achieve supercriticality (© Wikipedia and Cameron Reed) CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 17 Implosion design CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 18 Implosion design Explosive (fast) detonator detonation wave Explosive (slow) natural uranium tamper initiator Pu239 core high explosive blocks CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA Implosion design - Fat man CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 19 We doG not consider here density: theof role of inelastic scattering, differential for thediffusion neutron number ng bomb core,bomb the equation diffusion theory of Appendix provides sioning core, the theory Appendix G pr situation only indirectly in that it lowers the mean neutron vel al equation for the neutron number density: Critical Mass: Diffusion Theory " point with the eff @N v l v treatment simple we will talso not! deal2 at this ential equation for¼theneut neutron number density: neut ! " rN ; ð n # 1Þ N þ 20 l v N vneut @N lvt vneut tamper/neutron reflector. 2 neut ! 2 " t neut rnN#; 1lÞf N þ ðn # 1Þ N¼ þ (2.18) r N ¼ 3 @t ð ; core, the diffusion theory(2.18 In a spherical fissioning bomb of Ap lf 3 @t lf @t the following 3 differential equation for the neutron number dens neut neut 2 neutron velocity and the other symbols are as definedt earlier. the average neutronUpon velocity and erethevusual " neut is @N other vneut symbolsltare vneut !as2defin spherical radial coordinate. assuming a the r earlie ðnare # 1Þas Nþ N ; ¼ he average neutron velocity and the other symbols defined f e form N(t, Nt(t)Nr(r), (2.18) be separated as @t Now, letr)r¼represent thecanusual spherical radiallf coordinate.3 Upon as represent radial coordinate. Upon assuming $ # # spherical $& $ the %usual ution for r) N(t,vneut r)is¼ (2.18)and can be separat Nt n #N(t, 1 D of 1 @the 2form @Nr where the N average the other symbols a t(t)Nneutron r(r), velocity ¼ ; (2.19) þ r (t, r) oftthe form N(t, r) (2.18) can spherical be separated as Now, let rr(r), represent the usual radial coordinate. t(t)N @t @r ¼ N Nr r 2 @r # $ solution % form N(t,#r) ¼ Nt(t)N$r(r), & (2.18) can b # for $ N(t, r) of the D## $1 @# $&2$ @Nr % # $ 1 #@Nt $ n # %1 d diffusion# coefficient, $& ¼ ; þ r 1 @Nt n#1 D 1 @1 @N2t 2@Nrn # 1 D 1 @ 2 @Nr @t N¼ r ¼@r t ; þ@rN r2 @r r (2.19 þt t r 2 NN r t r @t lt vneut @r t r D ¼ ; (2.20) @r Nt @t 3 t Nr r @r where D is the so-called diffusion coefficient, ere D is the so-called diffusion coefficient, n time that a neutron will travel before causing a fission: e so-called diffusion coefficient, t r lt vneut 2 lf D¼ ; : mean time that a neutron (2.21) t¼ 3 2 l v vneut will travel before causing a fission t rD ¼ t neut ; lt vwhere neut t is the mean time that a neutron and willcoefficient travel before c Diffusion 3 @N v lv ð n # 1Þ N þ ¼ l 3 @t ! " rN ; erage neutron velocity and the other symbols are as defined esent the usual spherical radial coordinate. Upon assum of the form N(t, r) ¼ N (t)N (r), (2.18) can be separated # $ # % # $& $ @N n#1 D 1 @ @N ¼ ; þ r @t @r t N r @r D¼ ; (2.20 3 lf alled diffusion coefficient, : t¼ where t is the mean time that a neutron will travel before vneut causing a CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA separation a, but this will prove Note a littlethat more device is usedjust to initiate the form chain-reaction. we conve could sffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi ffi constant 21 equation must be equal), then the solution for the timeThe first and last terms in (2.23) can be combined (this where algebra. With this of the separation constant, themor rad separation constant justdefinition a, but this form will prove a little lf lsubsequent t constant was defined as a/t); on dividing (2.23) by D, we fin : (2.25) d¼ (2.19) appears as eutron density emerges directly as r subsequent algebra. With this definition of the separation constant, 3 ð $ a þ n $ 1Þ s ffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi ffi # ! "$ (2.26) x ¼ : (2.19) appears as 1 1 " 1 $@ # ! l!f lt " 2 @Nr d ða=tÞtd ¼ ¼ 0; r(2.25) n $ 1 : D 1 @ d2 þ2 @N a 2 r # r Nr !r @r¼ " $ w dimensionless coordinate If Nt ðtÞ þ " 2 (2.22) :@r ¼ No ex according as3 ð $ a þ tn $!1Þ n $N1r r @r D 1 @@r 2 @Ntr a ¼ : þ r where 2 the form r @r t Nr r @r t (2.26) ¼ :at e neutron density t ¼ 0. N would be set by whatever The first and last terms in (2.23) can be combined (this is why Now define ax new dimensionless coordinate x according as o sffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi ffi the s d lfind ! constant "$was f lt (this is wh defined a/t);terms on dividing (2.23) by D, we The firstwe andascould last in (2.23) can be combined e the # chain-reaction. Note that have called the : d¼ 1 1 @ @N 3ð $ a D, þ n we $ 1Þfind r r constant was defined 2 to the form as a/t); on dividing (2.23) by # ! " $ a, but this form a little convenient for ¼ $1: (2.27) x will prove (2.26) x ¼ :more 1 1 1 @ @N 2 r d 2 @x N x @x r # ! # ! " $ ¼ 0;"$ x according þdefine r Now a new dimensionless coordinate h this 1definition of the separation constant, the radial part of 2 2 1 @ 1 1 @@r 2 @Nr d Nr1 r @r 2 @Nr ¼ $1: (2.27) x ¼ 0; þ r 2 2 2 This brings (2.24) to the form @x Nr x @x @r r d Nr r @r ization constant, where the solution of this differential equation x ¼ d : # "$ ! "$ # ! " where constant, of1 this differential 1constant, @ the @Nr equation be 2 s(2.24) ffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi ffi nmalization $ Aside 1 from Da normalization 1 the@ solution @N a r This brings to the form 2 ¼ $1: x At the surface of the core (radius R) there will(2.27) be no “backflow” d to be 2 ¼ þ of this differential r : (2.23) solution equation is l l @x N x @x fffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi t the only neutrons r s ffi "that 2 of neutrons from the outside; # ! $ pass : d ¼ @r t Nr r !@r t ! " " 2.2 Critical Mass: Diffusion through the which have come 3surface ð $ of a the þ 1ncore $1lwill 1Þ lbet those r 2 @N Theory f@ sin x ¼ $1: x sin x : d ¼ from a characteristic distance λ from within 2 @x @x n $ r$ xa þ Aside from of this differential equation (2.28) NrrðrÞ :constant, the solution (2.28) N ðrÞa¼normalization ¼ x : 3 ðN! 1Þ " ! " ms in (2.23) can be combined (this is why the separation x can easily be verified to Now be define a new dimensionless coordinate 2 lt @N 2 as lt @N x according Aside from constant, N ðRCaÞ normalization ¼$ ¼ $the solution of :this a/t); on dividing (2.23) by D, we find 3coordinate 3 d @x as @r RC x according To determine a critical radius R C, we RC Now define a new dimensionless can easily be verified to be ! " ritical radius RC, we need a boundary condition to apply to r need a boundary condition sin x ✓ ◆! cal radius#G, RCthis , we need a boundary condition to apply to 2 : x ¼ in Appendix takes the form " ! "$Nr ðrÞ : (2.28) ¼ ⇥ D⇤ 2 sin x radius is d finds rthat On applying this to (2.28), one the critical Serber R = x 1 1 1 @ @N C : Nr:ðrÞ ¼ rthe form x ¼ 2 Appendix G, this takes 1 x the transcendental equation ¼ 0; (2.24) þ r d 2 2 @r @r FINELLI dCORSO N r This brings (2.24) to the form r DI FISICA NUCLEARE PAOLO FISICA ED ASTRONOMIA - UNIVERSITÀ DI to BOLOGNA To determine a critical radius R , we need aDIP.boundary condition to$ apply x cotðxÞ þ x=! 1 ¼ 0; Critical Mass: Diffusion Theory 22 Critical Mass Quantity A ρ σf σel ν n λfission λelastic λtotal RC MC Unit g/mol g/cm3 bn bn 1022 cm-3 cm cm cm cm kg CORSO DI FISICA NUCLEARE - PAOLO FINELLI 235U 239Pu 235,04 18,71 1,235 4,566 2,637 4,794 16,89 4,57 3,6 8,37 45,9 239,05 15,6 1,8 4,394 3,172 3,93 14,14 5,79 4,11 6,346 16,7 DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA eNbefore aDefine fission, is,separation as in (2.21): t; rÞ ¼ Nt that ðtÞ NdefinedðrÞ where tamp ðcausing the constant Nt a to ðtÞ and Nrepresent ðrÞ aremean respectively the here be d/t where t is the time that a r have to add term to (2.32) that effect. escaped back into the core; indeed, the modern name for a tamper is 23 and asubscripts tamp be usedin liberally neutron travel in the of coreNSuperscripts before causing fission,spherical that is, will as defined (2.21): here as it will be ; r is the usual radial coordinate. time-and space will dependences lcore fiss “reflector”, but I retain tamp the historical terminology here. This effect isboundary explored in t¼ : (2.34) necessary to join tamper physics to core physics via suitable conditions. v Upon substituting this into (2.32) we find, in analogy to (2.19), r neutrons Tamper - neutron reflector neut this section; estimating the distance over which the core expands before criticality lcore fiss as tEffect ¼the of : Tamper (2.34)is difficult to 2.3" no longer holds in taken up in next section. This slowing effect ! " ! # ! " $ The idea behindtamp a tamper is to surround the fissile core with atamp vneut tamp 1 @N l v 1 1 @an approximate @Nr " # model ! analytically, "$ neutbe treated with t 2 amp trans tamper tamp but can numerical model, which material. 1 of 1dense @ dThis serves two purposes: (i) it reduces ¼ : (2.33) r 2 @N rans vneutshell r tamp tamp ¼ : r (2.35) 2 @r in Sect. 2 @r choice @t 3 @rthe2.2, take a trial solution fo r As was done This renders (2.33) as 3 the @r r t N N Nrtamp is done in Sect. 2.5. r critical mass, and (ii) it slows the inevitable expansion of t tamp tamp tamp tamp The discussion here parallels that in Sect. 2.2. Neutrons that escape form the core core, allowing more time for fissions to occur until the core N ð t; r Þ ¼ N ðtÞ N ðrÞ where N ðtÞ and N ð core tamp ! with " !in the " # " $ t! t r r oke a core quantity when dealing diffusion tamp tamp tamp 1 @N l v 1 1 @ @N d neutrons neut Define the separation constant here to be d/t where t is the mean time that athetamper t 2 trans e separation constant however we please. In principle, r density will dropsdiffuse to the point where criticality no longer holds. into the tamper. To describe the behavior of in the ; r is usual sph time-and space dependences of N ¼ ¼ r : (2.35) tamp tamp tamp 2 exponential factor a of Sect. 2.2, but we will find that 3 @t @rto rfission, @r t Ncan Nr corresponding initiator The reduction in critical mass occurs because the tamper will t neutron will travel in the core before causing a that is, as defined in (2.21): we use (2.18) without the term production of neutrons, that is, to (2 Upon substituting this into (2.32) we find, in analogy that they be equal. This choice of separation constant some escaped neutrons back the core; the , which weterm assumeon to be same eutron reflect velocity vneut the first thetheright sideinto of (2.18); weindeed, are assuming that the tamper is not made It may seem strange to invoke a core quantity when dealing with diffusion in " the core . ! " ! # ! modernofname for a tamper is “reflector”, tamp tamp l material: fissconstant mean path 1 transport @N ltrans vneut (2.34) 1 1 @ pends on whether d isfissile positive, negative, or zero;the theseparation tamper, but we can define however we please. In principle, t free 2@ t ¼ : ¼ we will find that tamp 2 r threshold criticality in analogy to a ¼ 0 in Sect. 2.2. tamp v d may be different from the exponential factor a of Sect. 2.2, but neut N @t 3 r @r N terest will be d $ 0, in which case the solutions have r t tamp ! 2 of separation " ltransThis vneutchoice boundary conditions demand that@N they be equal. constant tamp ¼ v , which r Nassume (2.32) tamp ; to be the same we is advantageous that the velocity Fig. 2.5 Tamped bomb core neut This choice rendersin(2.33) asneutron @t 3separation constant here to be d/t where t Define the in both materials, þB ðd ¼ 0Þcancels out. neutron will travel in the core before causing a fission, tha tamp ! " ! " # ! " $ The solution of (2.35) depends on whether d is positive, negative, or zero; the (2.36) % r=d & tamp tamp number density of @and ltrans the transport mean free path for where Ntamp is the tamp e e&r=d 1 @N l v 1 1 @N d tÞt neut t ðdcorresponds 2 trans r to a ¼ 0 in Sect. 2.2. latter to threshold criticality in analogy þ B choice >¼ 0Þ; A r : the(2.35) neutrons in the tamper. v is the average neutron speed¼within tamper, which r tamp r neut tamp core 2 situations be dr $ @r 0, in which@rcase the solutions havelfiss @t of practical 3interest will t Nt Thewe N r will later assume for sake of simplicity to be the same as that within the core. t ¼ : the form of integration (different for the two cases), and where vneutwe would We are assuming that the tamper does not absorb neutrons; otherwise, sffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi 8 It may seem core strange to invoke a core quantity when dealing with diffusion in the have to add a term toA (2.32) represent that effect. ltamp l trans fiss > no constant absorption however ðwe > dtamp ¼ : can define the (2.37) þ B d(2.33) ¼please. 0Þ as In principle, tamper, but we separation > This choice renders 3 d Superscripts and < r subscripts tamp will be used liberally here as ✓ it will be ◆ sin(x/2) d may be different from the exponential factor a &r=d ofphysics Sect. but we will find that (2.36) N ¼ tamper % & 2.2, tamp necessary to join physics to core via suitable boundary conditions. r=d tamp tamp N" > e is that the neutron density in the core is described by r (r) = # e e! " ! ! > ð d=t Þt tamp tamp > boundary conditions demand:that they be equal. This choice of separation constant x þ B @Nt ðd > 0lÞ; e A 1 1 1 @ 2 @N trans vneut r r ¼ r we assume to be the same is advantageous in that the neutron velocity vtamp tamp neut, which 2 @t 3 @ r @r Nt Nr in both out. FINELLI CORSOmaterials, DI FISICA PAOLO DIP. FISICA ED ASTRONOMIA UNIVERSITÀ DI BOLOGNA where A NUCLEARE andcancels B are- constants of integration (different for the two cases), and -where tamp tamp Blast of atomic explosion Stokes, 19 kilotons, Nevada (57) CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 24 Blast of atomic explosion • Surface Blast: • Blast — 40-60% • Thermal radiation — 30-50% • Ionizing radiation — 5% • Residual radiation (fallout) — 5-10% surface destruction of structures through blast and firestorm, immediate radioactive fallout • High Altitude Air Blast: fireball > 100,000 ft (>3000m) interrupts satellite based communication through electromagnetic pulse (EMP) • Low Altitude Air Blast: fireball < 100,000 ft (without touching ground) generates shock waves • Subsurface Blast: Underwater burst generates surge Franklin, 4.7 kilotons, Nevada (57) CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 25 26 The fireball • Radiation release & absorption • Central temperature: ~10,000,000 K • Immediate vaporization of all material • Central pressure: ~3300 atm in surrounding matter generates red-glow intense luminosity. • Expansion of fireball through internal pressure • Fireball rises like hot air balloon Romeo, 11 megatons, Bikini atoll (54) CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA Fireball expansion 27 temperature pressure Qualitative temperature profiles are shown at the left and pressure profiles at the right of a series of photographs of the fireball at various intervals after the detonation of a 20 kiloton weapon. In the first picture, at 0.1 ms, the temperature is shown to be uniform within the fireball and to drop abruptly at the exterior, so that the condition is that of the isothermal sphere. Subsequently, as the shock front begins to move ahead of the isothermal sphere, the temperature is no longer uniform, as indicated by the more gradual fall near the outside of the fireball. In the isothermal stage, the pressure is uniform throughout and drops sharply at the outside, but after a short time, when the shock front has separated from the isothermal sphere, the pressure near the surface is greater than in the interior of the fireball. Within less than 1 ms the steep-fronted shock wave has traveled some distance ahead of the isothermal region. CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA The shock front development CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 28 29 The Mach Stem If the explosion occurs above the ground, when the expanding blast wave strikes the surface of the earth, it is reflected off the ground to form a second shock wave traveling behind the first. This reflected wave travels faster than the first, or incident, shock wave since it is traveling through air already moving at high speed due to the passage of the incident wave. The reflected blast wave merges with the incident shock wave to form a single wave, known as the Mach Stem. The overpressure at the front of the Mach wave is generally about twice as great as that at the direct blast wave front. At first the height of the Mach Stem wave is small, but as the wave front continues to move outward, the height increases steadily. At the same time, however, the overpressure, like that in the incident wave, decreases because of the continuous loss of energy and the ever-increasing area of the advancing front. After about 40 seconds, when the Mach front from a 1-megaton nuclear weapon is 10 miles from ground zero, the overpressure will have decreased to roughly 1 psi. CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 30 Overpressure Blast effects are usually measured by the amount of overpressure, the pressure in excess of the normal atmospheric value, in pounds per square inch (psi). After 10 seconds, when the fireball of a 1-megaton nuclear weapon has attained its maximum size (5,700 feet across), the shock front is some 3 miles farther ahead. At 50 seconds after the explosion, when the fireball is no longer visible, the blast wave has traveled about 12 miles. It is then traveling at about 784 miles per hour, which is slightly faster than the speed of sound at sea level. As a general guide, city areas are completely destroyed by overpressures of 5 psi, with heavy damage extending out at least to the 3 psi contour. CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 31 CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 32 CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 33 The mushroom CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 34 The mushroom Oak, 8.9 megatons, Enewetak atoll (58) • Absorption of cool air triggers fast toroidal circulation of hot gases and causes upward motion forming the stem and mushroom. • Strong upward wind drags dirt and debris into the cloud mixing with radioactive material • Cloud rises in height with ~ 440 ft/s CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 35 The mushroom the radioactive cloud CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 36 Altitude Maximum altitude for cloud rise is reached after ~ 6 min. CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA Airburst 37 3s 20 Kiloton air burst 0.5 s 10 s 1.25 s 30 s CORSO DI FISICA NUCLEARE - PAOLO FINELLI SURGE. A cloud which rolls outward from the bottom of the column produced by a subsurface explosion. For underwater bursts the visible surge is, in effect, a cloud of liquid (water) droplets. After the water evaporates, an invisible base surge of small radioactive particles may persist. DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 38 Airburst 30 s 30 s 0.5 s 10 s Shock-front fireball evolution Shock-front rebounce Surge and stem evolution Double shockfront upwards motion 1.25 s 3s CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA Mushroom from underwater tests CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 39 Surge & Cloud formation Cloud development 12 s Baker, Bikini atoll (1946) 23 kT Surge development 20 s 100 Kiloton shallow underwater burst CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 40 41 Cloud & fallout 1m Baker, Bikini atoll (1946) 23 kT 2.5 m 100 Kiloton shallow underwater burst CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 42 Cloud & fallout CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA Destructive Effects 1. Blast damage 2. Thermal damage 3. Radiation damage 4. EM-pulse 43 The generation of a mechanical shock through sudden increase of pressure causes mechanical damages The generation of a heat wave expanding with the shock causes incineration Electromagnetic shock leads to breakdown of communication systems CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA The mechanical shock 44 Dynamic pressure is the kinetic energy per unit volume of a fluid particle CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 45 Blast effects CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA from high static overpressure t winds. 46 Blast effects essure weakens Damage from highstructures static overpressure and blast winds. c pressure tears them apart. Static pressure weakens structures e/suction several seconds Dynamiclasts pressure tears them apart. Pressure/suction several seconds ces many timeslasts greater than the st hurricane. Exert forces many times greater than the strongest hurricane. ldings suffer moderate to severe atMost onlybuildings 5 psi! suffer moderate to severe damage at only 5 psi! from Burke, Kippenbrock and Young CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA Blast effects on humans CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 47 48 Nuclear firestorms Fires can result from combustion of dry, flammable debris set loose by the blast or from electrical short circuits, broken gaslines, etc. These fires can combine to form as terrible firestorm similar to those accompanying large forest fires. The intense heat of the fire causes a strong updraft, producing strong inward drawn winds in which fan the flame, take away oxygen so it is difficult to breath, and destroy everything in their path (Chimney Effect). Bluestone, 1.27 megatons, Christmas island (62) CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 49 Nuclear Firestorms Flash Blindness Caused by temporary bleaching of pigments in eyes Lasts around 40 min. Thermal Radiation Retinal Burns/Scarring Heat from direct viewing of fireball sears retinas, causing permanent damage. • Flash Burns Temperatures can Direct absorption of thermal energy intoexceed skin 100 million degrees C! Flame Burns (Thousands of times hotter Caused by contact with burning object than the surface of the sun) • • Matter immediately around device is vaporized. Fires ignited for miles around epicenter. Type 1 KT 20 KT Conflagratio 0.5 n 1 20 MT MT 2 10 30 3rd Deg. (skin loss) 0.6 2.5 12 38 2nd Deg. (blistering) 0.8 3.2 15 44 1st Deg. (sunburn) 1.1 4.2 19 53 from Burke, Kippenbrock and Young Range in km CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA Nuclear Radiation Radiation damage 50 Can be instantly Fatal instantly Fatal Radiation Sickness vomiting, diarrhea, hair loss,... on Nausea, Sickness: sea, vomiting, hea loss, fatigue, ures, coma juries occur explosion rm danger from Size of Device 1 20 KT KT Lethal total dose (neutrons and 0.8 1.4 gamma rays) Total dose for acute radiation syndrome 1.2 1.8 20 1 MT MT 2.3 4.7 2.9 5.4 Distance in km from Burke, Kippenbrock and Young CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA ElectroMagnetic Impulse (EMP) 51 Ionizing radiation from the fireball produces intense currents and electromagnetic fields, usually referred to as the electromagnetic pulse (EMP). This pulse is felt over very large distances. A single high-yield nuclear detonation will create destructive EMP over hundreds of thousands of square kilometers beneath where the explosion occurs. EMP from high-yield nuclear detonations will subject electrical grids to voltage surges far exceeding those caused by lightning. Modern chips and microprocessors, present in most communication equipment. TVs, radios, computers and other electronic equipment are extremely sensitive to these surges and immediately get burnt out. Thus all possible communication links to the outside world are cut off. Restoring these facilities will be an arduous (and expensive) task assuming that the infrastructure required to complete this task would still exist following a nuclear war. CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 52 The hydrogen bomb Mike, 10.4 megatons, Enewetak atoll (52) CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA The hydrogen bomb CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 53 54 6Li(n,t)4He CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA First application: booster D-T fusion can be used to increase (“boost”) the yield of a fission weapon With an equal mixture of D and T gas into the hollow cavity at the center of the pit made of NEM At the maximum compression of the pit, the temperature and density conditions in the interior can exceed the threshold for D+T fusion The D+T reaction releases only a very small amount of energy, but the resulting burst of 14 MeV neutrons initiates a new burst of fission reactions, greatly “boosting” the total fission yield of the weapon Advantages • Increases the maximum possible fission yield • Less hard-to-produce Pu or HEU is required for a given yield — the “efficiency” is higher • Warheads of a given yield can be smaller and lighter CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 55 Stanislaw Ulam CORSO DI FISICA NUCLEARE - PAOLO FINELLI Ed Teller DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 56 Andrej Dmitrievič Sacharov New Sloyka design by Sakharov Layer Cake: alternate layers of light (liquid deuterium and tritium) & heavy (235U) nuclear fuel to trigger a fission fusion reaction. In 1950 As “father” of the Soviet Hydrogen Bomb First design study by Andrei Sakharov CORSO DI FISICA NUCLEARE - PAOLO FINELLI Nobel Peace prize (1975) 1989, as regime dissident DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 57 Ulam-Teller design Staged explosion of fission (primary) bomb and fusion (secondary bomb). The fission bomb is based on a regular Pu-bomb design (Fat Man). Fusion device is based on d+d & d+t reaction with on-line 6Li(n,t) tritium production and n induced fission. The fusion bomb is triggered by rapid shock driven compression (Ulam) which is enhanced by radiation pressure (Teller) from released X-ray and γ-ray flux. CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 58 Ulam-Teller design CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 59 60 Ulam-Teller design CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 61 Ulam-Teller design 1) The fission bomb implodes, emitting X-rays 2) X-rays heat the interior of the bomb and the tamper, which prevents premature detonation of the fuel. The plastic foam between the radiation casing and secondary part which is essentially just carbon and hydrogen becomes completely ionized and transparent as the X-rays penetrate 3) The heat causes the tamper to expand and burn away, exerting pressure inward against the lithioum deuterate. The lithium deuterate is squeezed by about 1/30 of its original diameter, reaches or exceeds 1000 times its original density 4) The compression shock wave initiates fission in the plutonium rod CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 62 Ulam-Teller design 5) The fissioning rod gives off radiation, heat and neutrons. Fissionable rod experience an extremely violent shockwave that will heat it to high temperatures cause to compress and doing so increases its density by a factor of about 4 and cause the rod to become supercritical 6) The neutrons enter into the lithium deuterate and generate tritium. 7) The combination of high temperature and pressure is sufficient for tritiumdeuterium and deuterium-deuterium fusion reactions to occur, producing more heat, radiation and neutrons. 8) The neutrons from the fusion reactions induce fission in the U238 pieces from the tamper and shield. 9) Fission of the tamper and shield pieces produce even more radiation and heat 10) The bomb explodes. CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA Operation IVY, MIKE (31/10/1952) The "Mike" device was essentially a very large cylindrical thermos flask for holding the cryogenic deuterium fusion fuel, with a regular fission bomb (the "primary") at one end. The primary was a boosted fission bomb in a separate space atop the assembly. The "secondary" fusion stage used liquid deuterium because this fuel simplified the experiment. Running down the center of the flask which held it was a cylindrical rod of plutonium (the "sparkplug") to ignite the fusion reaction. Surrounding this assembly was a five-ton natural uranium "tamper". The interior of the tamper was lined with sheets of lead and polyethylene foam, which formed a radiation channel to conduct X-rays from the primary to secondary. The entire "Sausage" (as it was nicknamed) assembly measured 80 inches in diameter and 244 inches in height and weighed about 60 tons and weighed 82 tons. CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 63 Operation IVY, MIKE (31/10/1952) 10.4 Megatons — 577 more powerful than Nagasaki bomb CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 64 65 CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA Operation IVY, MIKE (31/10/1952) Before The blast created a crater 6,240 feet in diameter and 164 feet deep stripped the test islands clean of vegetation the water around the blast site boiled for up to twelve hours afterwards CORSO DI FISICA NUCLEARE - PAOLO FINELLI After DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 66 Operation CASTLE, BRAVO (1/3/1954) 15 Megatons, largest US H-bomb, solid fuel, 833 more powerful than Nagasaki bomb CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 67 68 CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA Operation CASTLE, BRAVO (1/3/1954) Castle Bravo was the most powerful nuclear device ever detonated by the United States, with a yield of 15 megatons. That yield, far exceeding the expected yield of 4 to 6 megatons, combined with other factors, led to the most significant accidental radiological contamination ever caused by the United States. Fallout from the detonation — intended to be a secret test — poisoned the islanders who had previously inhabited the atoll and returned there afterwards, as well as the crew of Daigo Fukuryū Maru (“Lucky Dragon No. 5″), a Japanese fishing boat. CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 69 The Bomb Test Programs CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 70 71 CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 72 Nuclear Detonation Timeline "1945-1998" http://www.youtube.com/watch?v=I9lquok4Pdk CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 73 CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 74 Greenhouse operation. First test with deuterium-tritium fusion via radiation process, in order to prepare Mike George, 225 kilotons, Enewetak atoll (51) CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 75 Plumbbob operation. Test for antinuclear buildings CORSO DI FISICA NUCLEARE - PAOLO FINELLI Priscilla, 37 kilotons, Nevada (57) DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 76 Plumbbob operation. Detonation in a hot-air balloon over Nevada military zone. Biggest bomb exploded over the U.S. land. CORSO DI FISICA NUCLEARE - PAOLO FINELLI Hood, 74 kilotons, Nevada (57) DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA Nuclear proliferation CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 77 78 CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA Acheson-Lilienthal Report (1946) Proposal of an Atomic Development Authority (ADA) in charge of the control of the whole field of atomic energy, from mining through manufacturing. Rather than rely on international inspection teams, the consultants proposed to control potential problem at the source, the uranium and thorium mines. The ADA was supposed to hand out and control fissionable material for peaceful use of nuclear energy. The Acheson-Lilienthal report recognized that with the fundamentals of atomic energy widely known, it was impossible to outlaw atomic weapons. It concluded that "so long as intrinsically dangerous activities may be carried out by nations, rivalries are inevitable" and that, therefore, a single international authority should become the only legal participant in activities associated with atomic arms. The report proposed that the US abandon its monopoly politics on nuclear weapons. CORSO DI FISICA NUCLEARE - PAOLO FINELLI Acheson Lilienthal DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 79 80 The Baruch Plan B. Baruch Baruch made two key changes in the Acheson-Lilienthal report that proved fatal. He insisted that swift and sure penalties greet violations and that punishment not be subject to a Security Council veto. Such conditions, Acheson believed, were a prescription for failure. The Soviet Union, a non-nuclear power, insisted upon retaining its United Nations veto and argued that the abolition of atomic weapons should precede the establishment of an international authority. Negotiations could not proceed fairly, the Russians maintained, as long as the United States could use its atomic monopoly to coerce other nations into accepting its plan. Gromyko Andrei Gromyko, the Soviet delegate, proposed an international convention prohibiting the possession, production, and use of nuclear weapons. Only after the convention was implemented, should measures be considered to ensure “the strict observance of the terms and obligations.” CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 81 CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA The Russell Einstein Manifesto (1955) "In view of the fact that in any future world war nuclear weapons will certainly be employed, and that such weapons threaten the continued existence of mankind, we urge the governments of the world to realize, and to acknowledge publicly, that their purpose cannot be furthered by a world war, and we urge them, consequently, to find peaceful means for the settlement of all matters of dispute between them." Max Born, Percy W. Bridgman , Albert Einstein, Leopold Infeld, Frederic Joliot-Curie, Herman J. Muller, Linus Pauling , Cecil F. Powell, Joseph Rotblat , Bertrand Russell, Hideki Yukawa CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 82 83 J. Foster Dulles Dwight “Ike” Eisenhower Massive Retaliation In the event of an attack from an aggressor, a state would massively retaliate by using a force disproportionate to the size of the attack. The aim of massive retaliation is to deter another state from initially attacking. For such a strategy to work, it must be made public knowledge to all possible aggressors. The aggressor also must believe that the state announcing the policy has the ability to maintain second-strike capability in the event of an attack, likely involving the use of nuclear weapons on a massive scale. CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA M.A.D. Mutual Assurance Destruction Mutually assured destruction, or mutual assured destruction (MAD), is a doctrine of military strategy and national security policy in which a full-scale use of high-yield weapons of mass destruction by two or more opposing sides would cause the complete annihilation of both the attacker and the defender. (“Nash equilibrium”) Robert S. McNamara CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 84 Comprehensive Nuclear-Test-Ban Treaty Partial Test Ban Treaty (1963) The treaty banned nuclear tests in the atmosphere, underwater and in space, but not underground. Neither France nor China signed the PTBT. However, the treaty was still ratified by the United States after an 80 to 19 vote in the United States Senate. The PTBT had no restraining effects on the further development of nuclear warheads. Nuclear Non-proliferation Treaty (1968) Under the NPT, non-nuclear weapon states were prohibited from, among other things, possessing, manufacturing or acquiring nuclear weapons or other nuclear explosive devices. All signatories, including nuclear weapon states, were committed to the goal of total nuclear disarmament. However, India, Pakistan and Israel have declined to sign the NPT on grounds that such a treaty is fundamentally discriminatory as it place limitations on states that do not have nuclear weapons while making no efforts to curb weapons development by declared nuclear weapons states. CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 85 Comprehensive Nuclear-Test-Ban Treaty Organization The Comprehensive Nuclear-Test-Ban Treaty Organization (CTBTO) is an international organization that will be established upon the entry into force of the Comprehensive NuclearTest-Ban Treaty, a Convention that outlaws nuclear test explosions. The organization will be tasked with verifying the ban on nuclear tests and will operate therefore a worldwide monitoring system and may conduct on site inspections. International Monitoring System (IMS) and Communications infrastructure The IMS, when completed, will consist of 1) 50 primary and 120 auxiliary seismic monitoring stations. 2) 11 hydro-acoustic stations detecting acoustic waves in the oceans. 3) 60 infra-sound stations using microbarographs (acoustic pressure sensors) to detect very lowfrequency sound waves. 4) 80 radionuclide stations using air samplers to detect radioactive particles released from atmospheric explosions and/or vented from underground or under-water explosions. 5) 16 radionuclide laboratories for analysis of samples from the radionuclide stations. CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 86 CTBTO: Signatures and Ratifications $%&$!%!'(%)*+(,,-..-("*/(%*'0& +(,$%&0&".-1&*"2+3&!%4'&.'45!" 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'%&!')*(%6!"-7!'-(" E BE BHG ($-"-("*("*'0&*$!%'*(/*'0&*J%(1-.-("!3*<&+0"-+!3 9&+%&'!%-!'*+("+&%"-"6*'0&*3&6!3*.'!'2.*(/*!") +(2"'%)K*'&%%-'(%)K*+-')*(%*!%&!*(%*-'.*!2'0(%-'-&.K (%*+("+&%"-"6*'0&*#&3-,-'!'-("*(/*-'.*/%("'-&%.*(% 5(2"#!%-&.> FB EG C ...8,&5&-8-(# E FF 8*9'!'&.*:0(.&*%!'-/-+!'-("*-.*%&;2-%&#*/(%*'0&*<%&!')*'(*&"'&%*-"'(*=(%+&> CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 87 A.B.M. AntiBallistic Missile An anti-ballistic missile (ABM) is a surface-to-air missile designed to counterballistic missiles (see missile defense). They are also used to deliver nuclear, chemical, biological or conventional warheads in a ballistic flight trajectory. The Anti-Ballistic Missile Treaty (ABM Treaty or ABMT, 1972) was a treaty between the United States and the Soviet Union on the limitation of the anti-ballistic missile (ABM) systems used in defending areas against ballistic missile-delivered nuclear weapons. Under the terms of the treaty, each party was limited to two ABM complexes, each of which were to be limited to 100 anti-ballistic missiles. CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 88 S.D.I. Strategic Defense Initiative CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 89 90 USA - URSS disarmament: chronology 1963: Limited Test Ban Treaty End of atmospheric testing “Hotline” Halt proliferation to other states 1967-1972: SALT I G. Ford and L. Brezhnev Set numerical limits on missile launchers (not warheads --> MIRVs) 1972-1979: SALT II Broader limits than SALT I…but Afghanistan spoiled negotiations 1972: ABM Treaty (AntiBallistic Missile Treaty) Limited each to two ABM sites (no nationwide defense) Prohibited sea-, air-, space-based systems Limit on qualitative improvement Problematic: “Star Wars”, US pull-out in 2001-2 M. Gorbacev and G. Bush 1972: Nuclear Nonproliferation Treaty 1987: INF treaty 1991: START I Treaty Negotiated almost 10 years Reductions in launchers (max. 1,600) and warheads (max. 6,000) V. Putin and G. Bush Jr. 1993: START II Treaty Further reductions; never ratified by US Senate and Russian Duma 2002: SORT (Strategic Offensive Reductions Treaty) Cut warheads to 1,700-2,200 by 2012 © Matt Rosenstein CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA A timeline of conflict, culture, and change CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 91 A timeline of conflict, culture, and change CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 92 A timeline of conflict, culture, and change CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 93 A timeline of conflict, culture, and change CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 94 A timeline of conflict, culture, and change CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 95 A timeline of conflict, culture, and change CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 96 A timeline of conflict, culture, and change CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 97 A timeline of conflict, culture, and change CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 98 A timeline of conflict, culture, and change CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 99 A timeline of conflict, culture, and change CORSO DI FISICA NUCLEARE - PAOLO FINELLI 100 DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA A timeline of conflict, culture, and change CORSO DI FISICA NUCLEARE - PAOLO FINELLI 101 DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA A timeline of conflict, culture, and change CORSO DI FISICA NUCLEARE - PAOLO FINELLI 102 DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA A timeline of conflict, culture, and change CORSO DI FISICA NUCLEARE - PAOLO FINELLI 103 DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA A timeline of conflict, culture, and change CORSO DI FISICA NUCLEARE - PAOLO FINELLI 104 DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA A timeline of conflict, culture, and change CORSO DI FISICA NUCLEARE - PAOLO FINELLI 105 DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA A timeline of conflict, culture, and change CORSO DI FISICA NUCLEARE - PAOLO FINELLI 106 DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA A timeline of conflict, culture, and change CORSO DI FISICA NUCLEARE - PAOLO FINELLI 107 DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA A timeline of conflict, culture, and change CORSO DI FISICA NUCLEARE - PAOLO FINELLI 108 DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA A timeline of conflict, culture, and change CORSO DI FISICA NUCLEARE - PAOLO FINELLI 109 DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA A timeline of conflict, culture, and change CORSO DI FISICA NUCLEARE - PAOLO FINELLI 110 DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA A timeline of conflict, culture, and change CORSO DI FISICA NUCLEARE - PAOLO FINELLI 111 DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 2015 CORSO DI FISICA NUCLEARE - PAOLO FINELLI 112 DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 113 CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA USA CORSO DI FISICA NUCLEARE - PAOLO FINELLI 114 DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 115 CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 116 CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 117 CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 118 CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 119 CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 120 USA Gorbachev and Reagan sign a treaty to ban all medium-range ballistic missiles (The INF Treaty) CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 121 © Limes CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA Russia ICBMs: 94 ICBM Launcher Pads: 54 Warheads: ~225 122 Belarus Ukraine ICBMs: 258 ICBM Launchers: 176 36 HBs: ~1,984 Warhead: ICBMs: 115 ICBM Launchers: 104 HBs: 40 Warhead:~1,462 Russia ICBMs: 1,340 SLBMs: 1,924 87 HBs: Warheads::~11,296 Kazakhstan SSBN Base ICBM Base (Silo) Mobile ICBM Base Production Facilities Non deployed ICBMs Heavy Bombers Major Destruction & Dismantlement Site Chemical Weapons & Support Facility CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA China CORSO DI FISICA NUCLEARE - PAOLO FINELLI 123 DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA France 124 Force de frappe - dissuasion du faible au fort - by Charles de Gaulle “Within ten years, we shall have the means to kill 80 million Russians. I truly believe that one does not light-heartedly attack people who are able to kill 80 million Russians, even if one can kill 800 million French, that is if there were 800 million French.” CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA Israel Vanunu worked at the Machon 2 facility, where plutonium is produced and bomb components fabricated, for 9 years before his increasing involvement in left wing pro-Palestinian politics led to his dismissal in 1986. Prior to his departure he managed to take about 60 photographs covering nearly every part of Machon 2. He made contact with the London Sunday Times which flew him to London and began preparing an exclusive news story. Unfortunately for Vanunu, the Israeli government had found out about his activities and the Mossad arranged to kidnap him and bring him back to Israel for trial. He was successfully lured into a trap by a female Israeli agent named Cheryl Bentov operating under the name of "Cindy". His sudden disappearance before the publication of the Sunday Times story was mysterious at the time. The story was finally published several days later on 5 October 1986. A few months later Vanunu's status as a prisoner of the Israeli government was confirmed when it was revealed that he would stand trial. 125 © www.nuclearweaponarchive.org/ Mordechai Vanunu CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA Israel Mordechai Vanunu CORSO DI FISICA NUCLEARE - PAOLO FINELLI Vanunu worked at the Machon 2 facility, where plutonium is produced and bomb components fabricated, for 9 years before his increasing involvement in left wing pro-Palestinian politics led to his dismissal in 1986. Prior to his departure he managed to take about 60 photographs covering nearly every part of Machon 2. He made contact with the London Sunday Times which flew him to London and began preparing an exclusive news story. Unfortunately for Vanunu, the Israeli government had found out about his activities and the Mossad arranged to kidnap him (via Rome) and bring him back to Israel for trial. He was successfully lured into a trap by a female Israeli agent named Cheryl Bentov operating under the name of "Cindy". His sudden disappearance before the publication of the Sunday Times story was mysterious at the time. The story was finally published several days later on 5 October 1986. A few months later Vanunu's status as a prisoner of the Israeli government was confirmed when it was revealed that he would stand trial. He was sentenced as a spy to 18 years in prison. He wrote «I’m Your Spy» early during the first 11 1/2 years he was held in strict isolation. He was released, with restrictions not to leave the country or talk with foreigners. He has been rearrested in 2007 and 2010 for violating his release terms. 126 DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA Israel I Am Your Spy 127 I am the clerk, the technician, the mechanic, the driver. They said, Do this, do that, don't look left or right, don't read the text. Don't look at the whole machine. You are only responsible for this one bolt. For this one rubber-stamp. This is your only concern. Don't bother with what is above you. Don't try to think for us. Go on, drive. Keep going. On, on. So they thought, the big ones, the smart ones, the futurologists. There is nothing to fear. Not to worry. Everything's ticking just fine. Our little clerk is a diligent worker. He's a simple mechanic. He's a little man. Little men's ears don't hear, their eyes don't see. We have heads, they don't. Answer them, said he to himself, said the little man, the man with a head of his own. Who is in charge? Who knows where this train is going? Where is their head? I too have a head. Why do I see the whole engine, Why do I see the precipice-- is there a driver on this train? The clerk driver technician mechanic looked up. He stepped back and saw -- what a monster. Can't believe it. Rubbed his eyes and -- yes, it's there all right. I'm all right. I do see the monster. I'm part of the system. I signed this form. Only now I am reading the rest of it. This bolt is part of a bomb. This bolt is me. How did I fail to see, and how do the others go on fitting bolts. Who else knows? Who has seen? Who has heard? -- The emperor really is naked. I see him. Why me? It's not for me. It's too big. Rise and cry out. Rise and tell the people. You can. I, the bolt, the technician, mechanic? -- Yes, you. You are the secret agent of the people. You are the eyes of the nation. Agent-spy, tell us what you've seen. Tell us what the insiders, the clever ones, have hidden from us. Without you, there is only the precipice. Only catastrophe. I have no choice. I'm a little man, a citizen, one of the people, but I'll do what I have to. I've heard the voice of my conscience and there's nowhere to hide. The world is small, small for Big Brother. I'm on your mission. I'm doing my duty. Take it from me. Come and see for yourselves. Lighten my burden. Stop the train. Get off the train. The next stop -- nuclear disaster. The next book, the next machine. No. There is no such thing. Mordechai Vanunu CORSO DI FISICA NUCLEARE - PAOLO FINELLI -1987, Ashkelon Prison DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA Israel 128 Terms of Release 1. he shall not be able to have contacts with citizens of other countries but Israel 2. his telephone and Internet use shall be monitored 3. he shall not own cellular phones 4. he shall not approach or enter embassies and consulates 5. he shall not come within 500 meters of any international border crossing 6. he shall not visit any port of entry and airport 7. he shall not leave the State of Israel Mordechai Vanunu CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 129 CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 130 I. Gandhi India 123-134 Lim QS bomba patil-sarkar:patil-sarkar 20-06-2012 11:40 Pagina 127 Smiling Buddha Test Crater L’INDIA NON FA PIÙ DA SOLA L’INDIA NUCLEARE Gilgit A QUALCUNO PIACE ATOMICA CINA PA K I S TA N 4 x700 Mw HARYANA Delhi RAJASTHAN Rawatbhata Kakrapar UTTAR PRADESH Bhopal BIHAR JHARKHAND 2 x700 Mw CH HA TTI SG AR H I N D I A 6 x1.000 Mw BHUTAN Lucknow MADHYA PRADESH 2 x700 Mw 2 x220 Mw N E PA L 2 x220 Mw Jaipur 2 x700 Mw 1 x100 Mw 1 x200 Mw 4x220 Mw Mithi Virdi SIKKIM Narora MAHARASHTRA IL PROGRAMMA NUCLEARE INDIANO IN 3 STADI ARUNACHAL PRADESH ASSAM MEGHALAYA NAGALAND PHWR MANIPUR Kolkata MIZORAM BENGALA (Calcutta) OCC. TRIPURA Haripur 6 x1.000 Mw Produzione di corrente elettrica Combustibile di uranio M YA N M A R Pu ORISSA Tarapur Mumbai (Bombay) 2 x160 Mw 4 x540 Mw Hyderabad 6 x1.650 Mw Jatapur ANDHRA PRADESH Panaji KA ATA RN Kaiga 4 x220 Mw ISOLE LACCADIVE Kavaratti Golfo del Bengala Th Pu Th FBR Produzione di corrente elettrica KA GOA Mare Arabico Kovada 6 x1.000 Mw ISOLE ANDAMANE Chennai (Madras) Port Blair 2x220 Mw KERALA OCEANO INDIANO Kudankulam 2 x1.000 Mw 223 U TAMIL NADU ISOLE NICOBARE 4 x1.000 Mw SRI LANKA Th Stati indiani che ospitano centrali nucleari 233 U Reattore nucleare autofertilizzante Reattori nucleari Attivi In costruzione Progetti lanciati nel 2010 Progetti proposti Impianti di arricchimento Fonte: Npcil; Global Fissile Material Report 2010. CORSO DI FISICA NUCLEARE - PAOLO FINELLI An Indian greeting card for Diwali from 1998, celebrating India’s nuclear tests. © http://tasveerghar.net 223 U Th Produzione di corrente elettrica 223 U Materiale in eccesso per uso militare © Limes Fonte: T.Woddi,W. Charleton, P. Nelson, India’s Nuclear Fuel Cycle: Unravelling the US-Indian Nuclear Accord, San Rafael Ca. 2009, Morgan and Cla DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA Pakistan CORSO DI FISICA NUCLEARE - PAOLO FINELLI 131 DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA Pakistan CORSO DI FISICA NUCLEARE - PAOLO FINELLI 132 DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 133 LA COREA ATOMICA North Korea IMPIANTI NUCLEARI P’yongyang: Laboratori per il processamento di materiale nucleare T’aech’on: Costruzione di un reattore atomico Yongbyon: Un vecchio reattore nucleare è stato rimesso in funzione nel 2003 e sembra che abbia prodotto tra le quattro e le sei bombe Sinp’o: Sito di reattori; attività interrotte nel 2003 Basi militari Aeree Navali Esercito Usa CINA NORD HAMGYONG CH‘ONGJIN Rang Hyesan YANGGANG P’UNGGYE-YOK YONG-CHO RI Kanggye MUSUDAN RI SANGNAM RI CHAGANG YOUNGDOKTONG SINUIJU NORD P’YONGAN COREA DEL NORD SITI DI TEST NUCLEARI Youngdoktong: Negli anni Novanta sembra ci siano state diverse forti esplosioni legate a test nucleari P’unggye-yok: Il 17 ottobre 2006 si è svolto un test nucleare sotterraneo SUD HAMGYONG SINP’O HAMBUNG YONGBYON T’AECH’ON TEYJO DONG SUD P’YONGAN PAKCH’ON SUNCHON P’yongyang SARIWON SUD HWANGHAE T’AETA’N Isola Baeknyeong Isola Yonp’yong L’AREA DELL’ULTIMO “INCIDENTE” TRA LE DUE COREE MISSILI BALISTICI Yong-cho Ri, Sangnam Ri: Impianti di lancio sotterranei Musudan Ri: Base di lancio del test per i missili Taedong 2 del 2006 WONSAN KANGWON NORD HWANGHAE P’YONGSAN KANGWON Ch’unch’on NUCHONRI KYONGGI KYONGGI KANGHWA MINIERE DI URANIO Sunchon: La miniera di uranio più grande P’yongsan: In attività a partire dagli anni Cinquanta Pakch’on: Miniera di uranio e impianto di estrazione KANGNUNG Seoul UIJONGBU SUWON YOUNGSAN CH’UNGCH’ONG © United States Geological Survey CHOONGWON Ch’ongju Taejon Mar Giallo FED. RUSSA KYONGSANG COREA DEL SUD KUNSAN DAEGU Mare dell’Est Chonju Ulsan Ch’angwon Kwangju Muan 0 SUNCH’ON KWANGJU Pusan © Limes 40 km POPOLAZIONE COREA DEL NORD 23.906.000 150 POPOLAZIONE COREA DEL SUD 50.062.000 © Limes Linea di cessate il fuoco Zona demilitarizzata fra le due Coree lunga 250 km e larga 4 km GIAPPONE Fonte: global.security.org.u.s. council on foreign relations, geohivue.com CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 134 CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA Iran CORSO DI FISICA NUCLEARE - PAOLO FINELLI 135 DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA Iran: an update 136 02/04/2015: speaking from the White House, President Obama announced details of a framework agreement between Iran and the P5+1—the United States, Russia, China, France, the United Kingdom, and Germany— that limits Iran’s path to building a nuclear weapon over the next 10 to 15 years. Although negotiators will finalize technical details between now and the June 30 deadline, the parameters provide Iran with sanctions relief in exchange for limits on its uranium enrichment, converting its Arak heavy water reactor, limiting the number and type of centrifuges, and agreeing to intrusive inspections. Should Iran cheat or fail to uphold its end of the bargain, however, the United States and its allies reserve the right to “snap-back” into place tough economic and financial sanctions. (© Washington Post) CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA Movies CORSO DI FISICA NUCLEARE - PAOLO FINELLI 137 DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 138 more pictures CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 139 Yankee, 13.5 megatons, Bikini atoll (54) CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA Frigate bird, 600 kilotons, Christmas island (62) CORSO DI FISICA NUCLEARE - PAOLO FINELLI 140 DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 141 Truckee, 210 kilotons, Christmas island (62) CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA Turk, 43 kilotons, Nevada (55) CORSO DI FISICA NUCLEARE - PAOLO FINELLI 142 DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 143 Xray, 37 kilotons, Enewetak atoll (48) CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 144 Met, 22 kilotons, Nevada (55) CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA Sugar, 1.2 kilotons, Nevada (51) CORSO DI FISICA NUCLEARE - PAOLO FINELLI 145 DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 146 Stokes, 19 kilotons, Nevada (57) CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 147 Laplace, 1 kiloton, Nevada (57) CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA Wheeler, 197 kilotons, Nevada (57) CORSO DI FISICA NUCLEARE - PAOLO FINELLI 148 DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA 149 Moth, 2 kilotons, Nevada (55) CORSO DI FISICA NUCLEARE - PAOLO FINELLI DIP. FISICA ED ASTRONOMIA - UNIVERSITÀ DI BOLOGNA