• No results found

Examination paper for TFY4225 Nuclear and Radiation Physics

N/A
N/A
Protected

Academic year: 2022

Share "Examination paper for TFY4225 Nuclear and Radiation Physics"

Copied!
10
0
0

Laster.... (Se fulltekst nå)

Fulltekst

(1)

Department of Physics

Examination paper for TFY4225 Nuclear and Radiation Physics

Academic contact during examination: Pål Erik Goa Phone: 959 08026

Examination date: 05.12.2016

Examination time (from-to): 9.00-13.00

Permitted examination support material (code C):

Simple specified calculator

Barnett & Cronin: Mathematical Formulae

Rottmann: Matematische Formelsammlung

Other information: Each sub-question (1, 2a, 2b etc) carries equal weight in the evaluation. Exam might be answered in English or Norwegian.

Language: English

Number of pages (front page excluded): 9

Checked by:

(2)

Note: Important information is given in tables, figures and equations after the problem text! Please browse through all sides before you start to work on the problems.

Problem 1

The nuclear shell model was a major step forward in nuclear physics.

• Describe the key ingredient of the model and how this a↵ected the output.

• What were the two main success-criteria for the model?

• Explain what is meant by the ”extreme independent particle model”.

• Give one example situation where the ”extreme independent particle model”

does not work.

Problem 2

11C can be used in positron emission tomography and can be produced in a cyclotron via the following reaction:

14N(p,↵)11C

The mass excess values for the particles involved are: 14N : 3074µu,1H : 7825µu,4He: 2603µu,11C: 11434µu.

Problem 2a

• Calculate the Q-value for the above nuclear reaction.

• Derive the expression for the required minimum (threshold) kinetic energy Tthof the proton in order for the reaction to occur.

• Calculate the numeric value ofTth.

Problem 2b

• Calculate the Coulomb barrier for the reaction (useR0= 1.6f m).

• Relate your results in 2a and 2b to the observed reaction cross-section as shown in figure 1, in particular the range 0-6 MeV.

(3)

Problem 2c

Production of11C:

• Set up the di↵erential equation for the number of11Cproduct nucleiN1(t), given a constant reaction rateR.

• Show that the expression forN1(t) given on the formula sheet is a solution to your equation, and calculate the irradiation time required to reach 90

% of maximum activity.

Problem 2d

The decay scheme of11Cis shown in figure 2.

• In the Fermi theory for beta-decay, explain the approximation behind what is called anallowed transition. Show that this approximation is justified.

• Explain/derive the selection rules for angular momentum and parity in the allowed approximation and explain why beta decay of 11C is an allowed transition.

• What is the di↵erence between a Fermi type and a Gamow-Teller type transition? Can you tell which type the 11C beta decay is? Justify your answer.

Problem 2e

A patient is injected with 1 GBq of11C for a PET exam. Assume even distri- bution of activity in the body and no biological clearance. Photon attenuation length in soft tissue @ 511 keV is 36 cm.

• Calculate the whole body e↵ective dose to the patient. If you need to make any further simplifying assumptions, please justify/explain them.

Problem 3

In figure 3 an example of a chain of events in a small volume of massdm= 1µgis shown. A photon of energyE = 662keV is Compton-scattered and an electron is released with initial kinetic energy Te= 100keV. This electron is scattered and a bremsstrahlung photon with energyEb= 20keV is emitted and leaves the volume. Via further interactions, the electron comes to rest within the volume.

• Calculate the energy imparted"and KERMA K for this example.

(4)

Problem 4

In the lab-assignments of this course we used two di↵erent detectors: a) NaI scintillator detector and b) HPGe (high-purity Germanium) semi-conductor de- tector.

• Describe the chain of events in the NaI scintillator detector from the initial interaction between the photon and the scintillator material to a count in the spectrum shown on the computer screen.

• Describe the chain of events in the HPGe detector.

• Describe how the output spectra from the two detectors will look. What is the key physical origin of the di↵erence between the two spectra?

Problem 5

The following 9 topics of ”Sources of Radiation” were covered in the first project work of this course:

1. Natural Radioactivity on Earth.

2. Radon Gas: focus on Norway.

3. Cosmic Radiation.

4. Medical Imaging Exams.

5. Chernobyl: Local Consequences and Europe in General.

6. Chernobyl: Consequences in Norway.

7. Fukushima Accident.

8. Low Dose Risk: Linear-No-Threshold Model.

9. Low Dose Risk: Hormesis Model.

Choose one of the above topics and describe what was presented on that topic.

Problem 6

The neutron absorption and scattering cross section for light water (H2O) and heavy water (D2O) is given in table 1. With respect to the neutron cycle in a thermal fission reactor, which type of water will give the highest neutron multiplication factor, given all other things equal? Justify your answer.

(5)

Table 1: Neutron absorption and scattering cross sections

Material a s

(b) (b) H2O 0.66 49.2 D2O 0.001 10.6

Figure 1: Reaction cross section for14N(p,↵)11C.

(6)

Figure 2: Decay scheme of11C.

(7)

Figure 4: Physical constants.

(8)

Appendix: Selected expressions

F = |q1q2| 4⇡✏0r2 P = q1q2

4⇡✏0r F~ = qE~ +q~v⇥B~

~

p = m~v L~ = ~r⇥~p F = ma F = mv2

r

U(~r) = Z ~r

1

F~ ·d~r

~ p(t) =

Z t 0

F d⌧~

T = 1 2mv2

p = mv

p1 v2/c2 E = p

p2c2+m2c4 T = E mc2 E0 = mc2

= h p p x  ~ 2 E t  ~ 2 Plane wave (x) = ei~p·~r/~

hl2i = ~2l(l+ 1) hlzi = ~ml

B = avA asA2/3 aCZ(Z 1)

A1/3 asym(A 2Z)2

A +

Q = X

mc2 X m c2

(9)

N(t) = N0e t A(t) ⌘ N(t)

t1/2 = ln2

=⌧ln2 N1(t) = R

1

(1 e 1t) N2(t) = N0

1

2 1

(e 1t e 2t)

= 2⇡

~ |Vf i|2⇢(Ef) Vf i =

Z

fV id⌫

= g2|Mf i| 2⇡~7c3

Z pmax

0

F(Z0, p)p2(Q Te)2dp

⇡(M L) = ( 1)L+1

⇡(EL) = ( 1)L pTb =

pmambTacos✓±p

mambTacos2✓+ (mY +mb) [mYQ+ (mY ma)Ta] mY +mb

sc =

X1 l=0

⇡¯(2l+ 1)|1 ⌘l|2

r =

X1 l=0

⇡¯(2l+ 1)(1 |⌘l|2)

dE dx =

✓ ze2 4⇡✏0

2

4⇡Z⇢NA

Amv2

 ln

✓2mv2 I

ln(1 2) 2 n = ⇢NA

A N = N0e µx

µ = n

= P E+Z C+ P P

D ⌘ d¯"

dm

" = Rin Rout+X Q dD

(10)

KC = E

✓µen

D(rT, TD) = X

rS

A(r˜ S, TD)S(rT rS)

S(rT rS) = 1 M(rT)

X

i

EiYi (rT rS, Ei)

A(r˜ S, TD) = Z TD

0

A(rS, t)dt

E = X

T

wT

X

R

wRDR(rT, TD)

Referanser

RELATERTE DOKUMENTER