Содержание

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Nuclear Physics Lectures

Cross-Sections

Why concept is important
Learn about dynamics of interaction and/or

Nuclear Physics Lectures Cross-Sections Why concept is important Learn about dynamics of
constituents (cf Feynman’s watches).
Needed for practical calculations.
Experimental Definition
How to calculate σ
Fermi Golden Rule
Breit-Wigner Resonances
QM calculation of Rutherford Scattering

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Nuclear Physics Lectures

Definition of σ

a+b?x
Effective area for reaction to occur is

Nuclear Physics Lectures Definition of σ a+b?x Effective area for reaction to
σ

Beam a

dx

Na

Na(0) particles type a/unit time hit target b
Nb atoms b/unit volume
Number /unit area= Nb dx
Probability interaction = σ Nbdx
dNa=-Na Nb dx σ
Na(x)=Na(0) exp(-x/λ) ; λ=1/(Nb σ)

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Nuclear Physics Lectures

Reaction Rates

Na beam particles/unit volume, speed v
Flux F= Na

Nuclear Physics Lectures Reaction Rates Na beam particles/unit volume, speed v Flux
v
Rate/target b atom R=Fσ
Thin target x<<λ: R=(NbT) F σTotal
This is total cross section. Can also define differential cross sections, as a function of reaction product, energy, transverse momentum, angle etc.
dR(a+b?c+d)/dE=(NbT) F dσ(a+b?c+d) /dE

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Nuclear Physics Lectures

Breit-Wigner Line Shape

Start with NR Schrödinger equation:

X by

Nuclear Physics Lectures Breit-Wigner Line Shape Start with NR Schrödinger equation: X
φ*n and integrate

Start in state m ? exponential decay

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Nuclear Physics Lectures

Breit-Wigner Line Shape - 2

For

Nuclear Physics Lectures Breit-Wigner Line Shape - 2 For

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Nuclear Physics Lectures

Breit-Wigner Line Shape -3

Normalised Breit-Wigner line shape

Q: where have

Nuclear Physics Lectures Breit-Wigner Line Shape -3 Normalised Breit-Wigner line shape Q:
you seen this shape before?
We will see this many times in NP and PP.

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Nuclear Physics Lectures

Breit-Wigner Resonance

Important in atomic, nuclear and particle physics.
Uncertainty relationship
Determine

Nuclear Physics Lectures Breit-Wigner Resonance Important in atomic, nuclear and particle physics.
lifetimes of states from width.
, Γ=FWHM;

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Nuclear Physics Lectures

Fermi Golden Rule

Want to be able to calculate reaction

Nuclear Physics Lectures Fermi Golden Rule Want to be able to calculate
rates in terms of matrix elements of H.
Warning: We will use this many times to calculate σ but derivation not required for exams, given here for completeness.

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Nuclear Physics Lectures

Discrete ? Continuum

Decays to a channel i (range

Nuclear Physics Lectures Discrete ? Continuum Decays to a channel i (range
of states n). Density of states ni(E). Assume narrow resonance

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Nuclear Physics Lectures

Cross Section

Breit Wigner cross section.
Definition of σ and flux

Nuclear Physics Lectures Cross Section Breit Wigner cross section. Definition of σ and flux F:
F:

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Nuclear Physics Lectures

Breit-Wigner Cross Section
Combine rate, flux & density states ?

Nuclear Physics Lectures Breit-Wigner Cross Section Combine rate, flux & density states ?

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Nuclear Physics Lectures

Breit-Wigner Cross Section

n + 16O? 17O

Nuclear Physics Lectures Breit-Wigner Cross Section n + 16O? 17O

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Nuclear Physics Lectures

Low Energy Resonances

n + Cd total cross section.
Cross section

Nuclear Physics Lectures Low Energy Resonances n + Cd total cross section.
scales σ ~ 1/E1/2 at low E.
B-W: 1/k2 and Γ~n(E)~k

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Nuclear Physics Lectures

Rutherford Scattering 1

Nuclear Physics Lectures Rutherford Scattering 1

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Nuclear Physics Lectures

Rutherford Scattering 2

Nuclear Physics Lectures Rutherford Scattering 2

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Nuclear Physics Lectures

Rutherford Scattering 3

Fermi Golden Rule:

Nuclear Physics Lectures Rutherford Scattering 3 Fermi Golden Rule:

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Nuclear Physics Lectures

Rutherford Scattering 4

Compare with experimental data at low energy
Q:

Nuclear Physics Lectures Rutherford Scattering 4 Compare with experimental data at low
what changes at high energy ?

pi

pf

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Nuclear Physics Lectures

Low Energy Experiment

Scattering of α on Au & Ag

Nuclear Physics Lectures Low Energy Experiment Scattering of α on Au &
? agree with calculation assuming point nucleus

Sin4(θ/2)

dN/dcosθ

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