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Introduction to Nuclei Physics 1 Wednesday, Mach, 23, 2011 Arif Hidayat 1. Nature of the Nuclear Force Shape of the Nuclear Potential Yukawa Potential Range of Yukawa Potential 2. Nuclear Models Liquid Drop Model Fermi Gas Model Shell Model

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Page 1: Model Model Inti

Introduction to Nuclei Physics

1

Wednesday, Mach, 23, 2011

Arif Hidayat

1. Nature of the Nuclear Force • Shape of the Nuclear Potential

• Yukawa Potential

• Range of Yukawa Potential

2. Nuclear Models • Liquid Drop Model

• Fermi Gas Model

• Shell Model

Page 2: Model Model Inti

• A square well nuclear potential provides the basis of quantum theory with discrete energy levels and corresponding bound state just like in atoms – Presence of nuclear quantum states have been confirmed

through • Scattering experiments • Studies of the energies emitted in nuclear radiation

• Studies of mirror nuclei and the scatterings of protons and neutrons demonstrate – Without the Coulomb effects, the forces between two

neutrons, two protons or a proton and a neutron are the same • Nuclear force has nothing to do with electrical charge • Protons and neutrons behave the same under the nuclear force

– Inferred as charge independence of nuclear force.

2

Nuclear Potential

Page 3: Model Model Inti

• Strong nuclear force is independent of the electric charge carried by nucleons – Concept of strong isotopic-spin symmetry.

• proton and neutron are the two different iso-spin state of the same particle called nucleon

– In other words, • If Coulomb effect were turned off, protons and neutrons

would be indistinguishable in their nuclear interactions

• Can you give another case just like this???

– This is analogues to the indistinguishability of spin up and down states in the absence of a magnetic field!!

• This is called Iso-spin symmetry!!!

3

Nuclear Potential – Iso-spin symmetry

Page 4: Model Model Inti

• EM force can be understood as a result of a photon exchange – Photon propagation is described by the Maxwell’s

equation – Photons propagate at the speed of light. – What does this tell you about the mass of the

photon? • Massless

• Coulomb potential is

• What does this tell you about the range of the Coulomb force? – Long range. Why?

4

Range of the Nuclear Force

V r 1

r

Massless

particle

exchange

Page 5: Model Model Inti

• For massive particle exchanges, the potential takes the form

– What is the mass, m, in this expression?

• Mass of the particle exchanged in the interaction – The force mediator mass

• This form of potential is called Yukawa Potential – Formulated by Hideki Yukawa in 1934

• What does Yukawa potential turn to in the limit m 0? – Coulomb potential

5

Yukawa Potential

V r

mcr

e

r

Page 6: Model Model Inti

• From the form of the Yukawa potential

• The range of the interaction is given by some characteristic value of r. What is this? – Compton wavelength of the mediator with

mass, m:

• What does this mean? – Once the mass of the mediator is known, range

can be predicted – Once the range is known, the mass can be

predicted 6

Ranges in Yukawa Potential

mcr

eV r

r

re

r

mc

Page 7: Model Model Inti

• Let’s put Yukawa potential to work • What is the range of the nuclear force?

– About the same as the typical size of a nucleus • 1.2x10-13cm

– thus the mediator mass is

• This is close to the mass of a well known p meson (pion)

• Thus, it was thought that p are the mediators of the nuclear force

7

Ranges in Yukawa Potential

2mc

mp

c

197164

1.2

MeV fmMeV

fm

2139.6 / ;MeV c

2

0 135 /m MeV cp

mp

Page 8: Model Model Inti

• Experiments showed very different characteristics of nuclear forces than other forces

• Quantification of nuclear forces and the structure of nucleus were not straightforward

– Fundamentals of nuclear force were not well understood

• Several phenomenological models (not theories) that describe only limited cases of experimental findings

• Most the models assume central potential, just like Coulomb potential

8

Nuclear Models

Page 9: Model Model Inti

• An earliest phenomenological success in describing binding energy of a nucleus

• Nucleus is essentially spherical with radius proportional to A1/3. – Densities are independent of the number of nucleons

• Led to a model that envisions the nucleus as an incompressible liquid droplet – In this model, nucleons are equivalent to molecules

• Quantum properties of individual nucleons are ignored

9

Nuclear Models: Liquid Droplet Model

Page 10: Model Model Inti

• Nucleus is imagined to consist of

– A stable central core of nucleons where nuclear force is completely saturated

– A surface layer of nucleons that are not bound tightly

• This weaker binding at the surface decreases the effective BE per nucleon (B/A)

• Provides an attraction of the surface nucleons towards the core just as the surface tension to the liquid

10

Nuclear Models: Liquid Droplet Model

Page 11: Model Model Inti

• If a constant BE per nucleon is due to the saturation of the nuclear force, the nuclear BE can be written as:

• What do you think each term does?

– First term: volume energy for uniform saturated binding

– Second term corrects for weaker surface tension

11

Liquid Droplet Model: Binding Energy

BE

• This can explain the low BE/nucleon

behavior of low A nuclei

– For low A nuclei, the proportion of the

second term is larger.

– Reflects relatively large number of

surface nucleons than the core.

1a A 2 3

2a A

Page 12: Model Model Inti

• Small decrease of BE for heavy nuclei can be understood as due to Coulomb repulsion – The electrostatic energies of protons have destabilizing

effect

• Reflecting this effect, the empirical formula for BE takes the correction term

• All terms of this formula have classical origin. • This formula does not explain

– Lighter nuclei with the equal number of protons and neutrons are stable or have a stronger binding (larger –BE)

– Natural abundance of stable even-even nuclei or paucity of odd-odd nuclei

• These could mainly arise from quantum effect of spins.

12

Liquid Droplet Model: Binding Energy

2 31 2BE a A a A 2 1 3

3a Z A

Page 13: Model Model Inti

• Additional corrections to compensate the deficiency, give corrections to the empirical formula (again…)

– All parameters are assumed to be positive

– The forth term reflects N=Z stability

– The last term • Positive sign is chosen for odd-odd nuclei, reflecting

instability

• Negative sign is chosen for even-even nuclei

• For odd-A nuclei, a5 is chosen to be 0.

13

Liquid Droplet Model: Binding Energy

2 3 2 1 31 2 3BE a A a A a Z A

2

4

N Za

A

3 45a A

Page 14: Model Model Inti

• The parameters are determined by fitting experimentally observed BE for a wide range of nuclei:

• Now we can write an empirical formula for masses of nuclei

• This is Bethe-Weizsacker semi-empirical mass formula

– Used to predict stability and masses of unknown nuclei of arbitrary A and Z

14

Liquid Droplet Model: Binding Energy

1 15.6a MeV 2 16.8a MeV 3 0.72 a MeV

4 23.3 a MeV 5 34 ; a MeV

2

, n p

BEM A Z A Z m Zm

c n pA Z m Zm

12

aA

c 2 32

2

aA

c 2 1 33

2

aZ A

c

2

42

N Za

Ac

3 452

aA

c

Page 15: Model Model Inti

• An early attempt to incorporate quantum effects

• Assumes nucleus as a gas of free protons and neutrons confined to the nuclear volume

– The nucleons occupy quantized (discrete) energy levels

– Nucleons are moving inside a spherically symmetric well with the range determined by the radius of the nucleus

– Depth of the well is adjusted to obtain correct binding energy

• Protons carry electric charge Senses slightly different potential than neutrons

15

Nuclear Models: Fermi Gas Model

Page 16: Model Model Inti

• Nucleons are Fermions (spin ½ particles) so – Obey Pauli exclusion principle – Any given energy level can be occupied by at most

two identical nucleons – opposite spin projections

• For a greater stability, the energy levels fill up from the bottom to the Fermi level – Fermi level: Highest, fully occupied energy level (EF)

• Binding energies are given as follows: – BE of the last nucleon= EF since no Fermions above

EF – In other words, the level occupied by Fermion

reflects the BE of the last nucleon

16

Nuclear Models: Fermi Gas Model

Page 17: Model Model Inti

• Experimental observations show BE is charge independent

• If the well depth is the same for p and n, BE for the last nucleon would be charge dependent for heavy nuclei (Why?)

– Since there are more neutrons than protons, neutrons sit higher EF

17

Nuclear Models: Fermi Gas Model

Page 18: Model Model Inti

Same Depth Potential Wells

18

Neutron Well Proton Well

Nuclear b-decay

nFE

pFE…

en e p

Page 19: Model Model Inti

• Experimental observations show BE is charge independent • If the well depth is the same for p and n, BE for the last

nucleon would be charge dependent for heavy nuclei (Why?) – Since there are more neutrons than protons, neutrons sit higher

EF

– But experiments observed otherwise • EF must be the same for protons and neutrons. How do

we make this happen? – Make protons move to a shallower potential well

19

Nuclear Models: Fermi Gas Model

• What happens if this weren’t the

case?

– Nucleus is unstable.

– All neutrons at higher energy levels

would undergo a b-decay and

transition to lower proton levels

Page 20: Model Model Inti

• Fermi momentum: • Volume for momentum space up to Fermi level • Total volume for the states (kinematic phase space)

– Proportional to the total number of quantum states in the system

• Using Heisenberg’s uncertainty principle: • The minimum volume associated with a physical

system becomes • The nF that can fill up to EF is

20

3

22

TOTF

Vn

p

Fermi Gas Model: EF vs nF

2F Fp mE

FpV

FTOT pV V V

x p

3

2stateV p

30

4

3r A

p

23

0

4

3FA r p

p

23

03

2 4

32FA r p

p

p

3

04

9

Fr pA

p

2 2F FE p m

34

3Fp

p

34

3Fp

p

2

Why?

Page 21: Model Model Inti

• Let’s consider a nucleus with N=Z=A/2 and assume that all states up to Fermi level are filled

• What do you see about pF above? – Fermi momentum is constant, independent of the number

of nucleons

• Using the average BE of -8MeV, the depth of potential well (V0) is ~40MeV – Consistent with other findings

• This model is a natural way of accounting for a4 term in Bethe-Weizsacker mass formula

21

Fermi Gas Model: EF vs nF

2

AN Z

1 3

0

9

8Fp

r

p

or

FE

3

04

9

Fr pA

p

2

2

Fp

m

2 2 3

0

1 9

2 8m r

p

2

20

2.32

2

c

rmc

2.32 19733

2 940 1.2

MeV fmMeV

fm

Page 22: Model Model Inti

• Exploit the success of atomic model

– Uses orbital structure of nucleons

– Electron energy levels are quantized

– Limited number of electrons in each level based on available spin and angular momentum configurations • For nth energy level, l angular momentum (l<n), one

expects a total of 2(2l+1) possible degenerate states for electrons

22

Nuclear Models: Shell Model

Page 23: Model Model Inti

• Orbits and energy levels an electron can occupy are labeled by – Principle quantum number: n

• n can only be integer

– For given n, energy degenerate orbital angular momentum: l • The values are given from 0 to n – 1 for each n

– For any given orbital angular momentum, there are (2l+1) sub-states: ml

• ml=-l, -l+1, …, 0, 1, …, l – l, l

• Due to rotational symmetry of the Coulomb potential, all these sub-states are degenerate in energy

– Since electrons are fermions w/ intrinsic spin angular momentum , • Each of the sub-states can be occupied by two electrons

– So the total number of state is 2(2l+1) 23

Atomic Shell Model Reminder

2

Page 24: Model Model Inti

• Exploit the success of atomic model

– Uses orbital structure of nucleons

– Electron energy levels are quantized

– Limited number of electrons in each level based on available spin and angular momentum configurations • For nth energy level, l angular momentum (l<n), one expects a

total of 2(2l+1) possible degenerate states for electrons

• Quantum numbers of individual nucleons are taken into account to affect the fine structure of spectra

24

Nuclear Models: Shell Model

Page 25: Model Model Inti

• Nuclei have magic numbers just like inert atoms

– Atoms: Z=2, 10, 18, 36, 54

– Nuclei: N=2, 8, 20, 28, 50, 82, and 126 and Z=2, 8, 20, 28, 50, and 82

– Magic Nuclei: Nuclei with either N or Z a magic number Stable

– Doubly magic nuclei: Nuclei with both N and Z magic numbers Particularly stable

• Explains well the stability of nucleus

25

Nuclear Models: Shell Model

Page 26: Model Model Inti

• To solve equation of motion in quantum mechanics, Schrödinger equation, one must know the shape of the potential

– Details of nuclear potential not well known

• A few shapes of potential energies tried out

– Infinite square well: Each shell can contain up to 2(2l+1) nucleons

26

Shell Model: Various Potential Shapes

2

2

20

mE V r r

Page 27: Model Model Inti

27

Nuclear Models: Shell Model – Square

well potential case

NM n l=n-1 Ns=2(2l+1) NT

2 1 0 2 2

8 2 0,1 2+6 8

20 3 0,1,2 2+6+10 18

28 4 0,1,2,3 2+6+10+14 32

50 5 0,1,2,3,4 2+6+10+14+18 50

82 6 0,1,2,3,4,5 2+6+10+14+18+22 72

Page 28: Model Model Inti

• To solve equation of motion in quantum mechanics, Schrödinger equation, one must know the shape of the potential

– Details of nuclear potential not well known

• A few models of potential tried out

– Infinite square well: Each shell can contain up to 2(2l+1) nucleons

• Can predict 2, 8 and 50 but no other magic numbers

– Three dimensional harmonic oscillator:

• Predicts 2, 8, 20, 40 and 70 Some magic numbers predicted

28

Shell Model: Various Potential Shapes

V r 2 21

2m r

2

2

20

mE V r r

Page 29: Model Model Inti

• Central potential could not reproduce all magic numbers

• In 1940, Mayer and Jesen proposed a central potential + strong spin-orbit interaction w/

– f(r) is an arbitrary empirical

function of radial coordinates and chosen to fit the data

• The spin-orbit interaction with the properly chosen f(r), a finite square well can split

• Reproduces all the desired magic numbers

29

Shell Model: Spin-Orbit Potential

TOTV

Spectroscopic notation: n L j

Orbit number Orbital angular

momentum Projection of

total momentum

V r f r L S

Page 30: Model Model Inti

• Spin-Parity of large number of odd-A nuclei predicted well – Nucleons are Fermions so the obey Pauli exclusion

principle

– Fill up ground state energy levels in pairs

– Ground state of all even-even nuclei have zero total angular momentum

• The shell model cannot predict stable odd-odd nuclei spins – No prescription for how to combine the unpaired

proton and neutron spins

30

Predictions of the Shell Model

Page 31: Model Model Inti

• Magnetic Moment of neutron and proton are

• Intrinsic magnetic moment of unpaired nucleons contribute to total magnetic moment of nuclei

– What does a deuteron consist of?

• Measured value is

– For Boron (10B5) , the 5 neutrons and 5 protons have the same level structure: (1S1/2)2(1P3/2)3, leaving one of each unpaired proton and neutron in angular momentum l=1 state

• Measured value is

• Does not work well with heavy nuclei 31

Predictions of the Shell Model

D

2.79p N 1.91n N

D

B

1.80B N

2.79 1.91N N N

p 2.79 N 1.91 N 0.88 Nn

0.86 N

2 N

el

m c N1

2 N

e

m c

p n orbit 1.88 N

Page 32: Model Model Inti

• For heavy nuclei, shell model predictions do not agree with experimental measurements – Especially in magnetic dipole moments

• Measured values of quadrupole moments for closed shells differ significantly with experiments – Some nuclei’s large quadrupole moments suggests

significant nonspherical shapes – The assumption of rotational symmetry in shell model

does not seem quite right

• These deficiencies are somewhat covered through the reconciliation of liquid drop model with Shell model – Bohr, Mottelson and Rainwater’s collective model,

1953 32

Collective Model

Page 33: Model Model Inti

• Assumption – Nucleus consists of hard core of nucleons in filled shells – Outer valence nucleons behave like the surface molecules in a

liquid drop – Non-sphericity of the central core caused by the surface motion of

the valence nucleon

• Thus, in collective model, the potential is a shell model with a spherically asymmetric potential – Aspherical nuclei can produce additional energy levels upon

rotation while spherical ones cannot

• Important predictions of collective model: – Existence of rotational and vibrational energy levels in nuclei – Accommodate decrease of spacing between first excite state and

the ground level for even-even nuclei as A increases, since moment of inertia increases with A

– Spacing is largest for closed shell nuclei, since they tend to be spherical

33

Collective Model

Page 34: Model Model Inti

• Nuclei tend to have relatively small intrinsic spins

• Particularly stable nuclei predicted for A between 150 and 190 with spheroidal character – Semi-major axis about a factor of 2 larger than semi-minor

• Heavy ion collisions in late 1980s produced super-deformed nuclei with angular momentum of

• The energy level spacings of these observed through photon radiation seem to be fixed

• Different nuclei seem to have identical emissions as they spin down

• Problem with collective model and understanding of strong pairing of nucleon binding energy

• Understanding nuclear structure still in progress 34

Super-deformed Nuclei

60