p3 week 9 - relativity and nuclear fission

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    Specialrelativity

    Specialrela*vitypostulate1:

    Thelawsofphysicsholdtrueforallframesofreference.Specialrela*vitypostulate2:

    Thespeedoflightisaconstantforallframesofreference.

    c

    u

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    Specialrelativity:Length

    Contraction Objectstravellingclosetothespeedoflightseemtocontractinthedirec*onofmo*on

    x

    y

    z

    x'

    y'

    z'

    L = L01

    v2

    c2

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    Specialrelativity:Time

    Dilation Timeisnotanabsolutequan*ty.Itisrela*ve Forobjectsmovingclosetothespeedoflight*meseemstorunslower

    t=t0

    1v2

    c2

    x

    y

    z

    x'

    y'

    z'

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    Thetwinparadox

    Ifyouhadatwinandwhenyouwereboth20youboardedonaspaceshiptravellingat95%thespeedoflightwhilethey

    stayedhereonEarthwhileyoutravelledfor25years(as

    measuredbyyourclock)andcamebackwhenyouwere45,

    howoldwouldyourtwinbe?

    t=t0

    1

    v

    2

    c2

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    Relativisticmass

    Rest(orinvariant)mass=invariantquan*ty,sameinallreferenceframes

    Rela*vis*cmass=dependentonthevelocityoftheobserver Theincreaseineffec*vemasswithspeedisgivenby

    Rela*vis*cmassisatermusedwhenspeakingaboutthetotalenergyofasystem.

    mr=

    m0

    1v2

    c2

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    Massandenergy

    TheenergyE(inJoules)producedbyachangeofmassm(inkg)isgivenby

    Wherec=speedoflight=3108m/s InnuclearphysicstheeVismorecommonlyusedastheunitofenergy:1eV=1.610-19J

    1MeV=1.610-13J

    E=mrc2

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    Example

    When1kgofwaterabsorbs4.2103Jofenergytoproducea

    temperaturechangeof1K.Whatistheincreaseinthemassofthe

    water?

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    Example

    Ifthemassdecreasemforthedecayof1atomofradiumis

    8.6x10-30kg,howmuchenergyisreleased?

    88

    226Ra

    2

    4He+

    86

    222Rn

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    Uni?iedatomicmass

    Energycanalsobeexpressedintermsofmass Theunifiedatomicmassunit(u)isdefinedas1/12ththemassofthecarbonatom

    Howmassiveis1u? 1u=1.6610-27kg 1u=931MeV

    6

    12C

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    BindingEnergy

    Theprotonsandneutronsinthenucleusofanatomarecallednucleons

    Theworkofenergyneededtotakethenucleonsapartiscalledthebindingenergyof

    thenucleus Itistheenergyassociatedwiththestrongnuclearforce

    Themassdefect(ormassdifference)ofanucleusisdefinedasthedifferencebetweenthemassoftheseparatednucleonsandthe

    combinedmassofthenucleus

    Thebindingenergyistheenergyequivalentofthemassdifference(E=mc2)

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    NuclearForcesandBinding

    Energy Thesearetheforceskeepingatomicnucleitogether Theyarealwaysarac*ve Theyhaveaveryshortrange(oftheorderof2-3femto-meters(x10-15))

    Anucleuswithanucleonnumber(massnumber)(N+Z)andaproton(atomicnumber)ZhasZprotonsandNneutrons

    BindingenergyofatomBindingenergy=massofNneutrons+massofZprotonsmassofnucleus

    atlessthan0.5fmthenuclearforceisrepulsivesothenucleonsdonottouch

    Z

    N+ZX

    Z

    N+ZX

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    Example

    AHeliumnucleushas4nucleons,2protonsand2neutrons.The

    massofaprotonis1.0073uandthemassofaneutronis1.0087

    u.IfthemassoftheHeliumnucleusis4.0015u,whatis

    a)thebindingenergyofthenucleusinMeV?

    b)thebindingenergypernucleoninMeV?

    (1u=931MeV)

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    Bindingenergycurve

    Fusion

    Fission

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    Energyofdisintegration

    Consideraradioac*vedecayprocessby-par2cleemission

    atomicmasses:

    Before:211.99127u 83me

    Aer:(207.98201u 81me)+(4.002604u 2m

    e)

    Massloss:(totalmassbefore)(totalmassaer)=(211.99127u 83m

    e)

    (207.98201u 81m

    e+4.002604u 2

    me)=0.006656u =6.2MeV

    83

    212Bi

    2

    4He+

    81

    208Tl +Q

    83

    212Bi = 211.99127u

    2

    4He = 4.002604u 81

    208Tl = 207.98201u

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    Energyofdisintegration

    Consideraradioac*vedecayprocessby-par2cleemission

    atomicmasses:

    Before:89.90730u -38me

    Aer:(89.90670u 39me)+m

    e

    Massloss:(totalmassbefore)(totalmassaer)=(89.90730u 38m

    e)

    (89.90670u 39m

    e+m

    e)=0.00060u =

    0.56MeV

    38

    90Sr

    1

    0e+

    39

    90Y+ v+Q

    38

    90Sr = 89.90730u

    1

    0e = 0.00055u =m

    e 39

    90Y = 89.90670u

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    Energyofdisintegration

    Consideraradioac*vedecayprocessby+-par2cleemission

    atomicmasses:

    Before:29.97832u -15me

    Aer:(29.97376u 14me)+m

    e

    Massloss:(totalmassbefore)(totalmassaer)=(29.97832u 15m

    e)

    (29.97376u 13m

    e)=0.00456u

    20.00055u =0.00346u =3.22MeV

    15

    30P

    +1

    0e+

    14

    30Si++Q

    15

    30P = 29.97832u

    +1

    0e = 0.00055u =m

    e 14

    30Si = 29.97376u

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    Nuclear?ission

    Fissionhappenswhenaheavyatomicnucleussplitsintotwolighternuclei

    Thenucleusisdeeplydividedintotwolargefissionfragmentsofroughlyequalmass

    Themassdecrease(andhencetheenergyreleased,Q)isappreciable

    Otherneutronsareemiedintheprocess(calledfissionneutrons)

    92

    235U+

    0

    1n

    56

    144Ba+

    36

    90Kr + 2

    0

    1n+Q

    Chainreac2on:fissionneutronsproducefurtherfission

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    ToDo

    Readchapter30[p.614-626NuclearEnergy]