# Difference between revisions of "Forest NucPhys I"

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Neutrino | Neutrino | ||

+ | |||

+ | :<math>\nu_e + {40 \atop 18 }Ar_{22} \rightarrow {40 \atop 19 }K^*_{21} + e^- </math> | ||

+ | |||

+ | The min neutrino energy needed for this reaction assuming the electron energy is ignorable: | ||

+ | |||

+ | :<math>\Delta M = \left [ m\left({40 \atop 19 }K\right)- m\left({40 \atop 18 }Ar\right) \right] c^2 </math> | ||

+ | : <math>= \left [ 39.96399848 - 39.9623831225 \right] 931.502 \frac{\mbox{MeV}}{\mbox {u}} </math> | ||

+ | :<math>= 0.00162 931.502 \frac{\mbox{MeV}}{\mbox {u}} = 1.505 MeV</math> | ||

+ | |||

+ | A reaction to the ground state of potassium is forbidden in this charged current electron neutrino reaction resulting in one or more gammas being emitted as the Potassium nucleus de-excited to the ground state. There are about 98 observed excited states of the K-40 nucleus. | ||

+ | |||

+ | Detecting this signal in DUNE means you need to see and electron and at least one gamma in coincidence. | ||

Potassium 40 decay | Potassium 40 decay | ||

Line 287: | Line 299: | ||

Argon-39 decay: | Argon-39 decay: | ||

− | :<math>{39 \atop 18 }Ar_{21} \rightarrow {39 \atop 19 }K_{20} + e^- + \nu</math> | + | :<math>{39 \atop 18 }Ar_{21} \rightarrow {39 \atop 19 }K_{20} + e^- + \bar{\nu}</math> |

=Strong Interaction= | =Strong Interaction= |

## Latest revision as of 01:07, 18 December 2015

Advanced Nuclear Physics

- References:
- Introductory Nuclear Physics
- Kenneth S. Krane: ISBN 9780471805533

Catalog Description:

PHYS 609 Advanced Nuclear Physics 3 credits. Nucleon-nucleon interaction, bulk nuclear structure, microscopic models of nuclear structure, collective models of nuclear structure, nuclear decays and reactions, electromagnetic interactions, weak interactions, strong interactions, nucleon structure, nuclear applications, current topics in nuclear physics. PREREQ: PHYS 624 OR PERMISSION OF INSTRUCTOR.

PHYS 624-625 Quantum Mechanics 3 credits. Schrodinger wave equation, stationary state solution; operators and matrices; perturbation theory, non-degenerate and degenerate cases; WKB approximation, non-harmonic oscillator, etc.; collision problems. Born approximation, method of partial waves. PHYS 624 is a PREREQ for 625. PREREQ: PHYS g561-g562, PHYS 621 OR PERMISSION OF INSTRUCTOR.

# NucPhys_I_Syllabus

# Introduction

The interaction of charged particles (electrons and positrons) through the exchange of photons is described by a fundamental theory known as Quantum ElectroDynamics(QED). QED has perturbative solutions which are limited in accuracy only by the order of the perturbation you have expanded to. As a result, the theory is quite useful in describing the interactions of electrons that are prevalent in Atomic physics.

Nuclear physics describes how Atomic nuclei interact via the strong forces as well as how the strong force binds the constituents of a nucleus (protons and neutrons, a.k.a. nucleons). Particle physics studies the interactions of fundamental particles, particles without substructure like quarks, photons, and electrons. Both Nuclear and Particle physics rely on the "Standard Model", a field theory description of the strong, weak and electromagnetic forces. Quantum ChromoDynamic (QCD) is one component to the Standard Model which represents the fundamental theory developed to describe the interactions of the quarks and gluons inside a nucleon, analogous to how QED describes the electromagnetic forces of electrons within the atom. The electroweak and Higgs field are the remaining components to the Standard model.
Ideally, QCD is a field theory which could be used to describe how quarks interact to for nucleons and then describe how those nucleons interact to form a nucleus and eventually lead to a description of how the nucleus interacts with other nuclei.
Unfortunately, QCD does not have a complete solution at this time. At very high energies, QCD can be solved perturbatively. This is an energy at which the strong coupling constant is less than unity where

The objectives in this class will be to discuss the basic aspects of the nuclear phenomenological models used to describe the nucleus of an atom in the absence of a QCD solution.

## Nomenclature

Variable | Definition |

Z | Atomic Number = number of protons in an atom |

A | Atomic Mass |

N | number of neutrons in an atom = A-Z |

Nuclide | A specific nuclear species |

Isotope | Nuclides with same Z but different N |

Isotones | Nuclides with same N but different Z |

Isobars | Nuclides with same A |

Nuclide | A specific nuclear species |

Nucelons | Either a neutron or a proton |

J | Nuclear Angular Momentum |

angular momentum quantum number | |

s | instrinsic angular momentum (spin) |

total angular momentum = | |

Spherical Harmonics, | = angular momentum quantum number, = projection of on the axis of quantization|

Planks constant/2 |

### Notation

= An atom identified by the Chemical symbol with protons and neutrons.

Notice that

and are redundant since can be identified by the chemical symbol and can be determined from both and the chemical symbol (N=A-Z).- example

## Historical Review

### Rutherford Nuclear Atom (1911)

Rutherford interpreted the experiments done by his graduate students Hans Geiger and Ernest Marsden involving scattering of alpha particles by the thin gold-leaf. By focusing on the rare occasion (1/20000) in which the alpha particle was scattered backward, Rutherford argued that most of the atom's mass was contained in a central core we now call the nucleus.

### Chadwick discovers neutron (1932)

Prior to 1932, it was believed that a nucleus of Atomic mass

was composed of protons and electrons giving the nucleus a net positive charge . There were a few problems with this description of the nucleus- A very strong force would need to exist which allowed the electrons to overcome the coulomb force such that a bound state could be achieved.
- Electrons spatially confined to the size of the nucleus ( would have a momentum distribution of . Electrons ejected from the nucleus by radioactive decay ( decay) have energies on the order of 1 MeV and not 20.
- Deuteron spin: The total instrinsic angular momentum (spin) of the Deuteron (A=2, Z=1) would be the result of combining two spin 1/2 protons with a spin 1/2 electron. This would predict that the Deuteron was a spin 3/2 or 1/2 nucleus in contradiction with the observed value of 1.

The discovery of the neutron as an electrically neutral particle with a mass 0.1% larger than the proton led to the concept that the nucleus of an atom of atomic mass

was composed of protons and neutrons.### Powell discovers pion (1947)

Although Cecil Powell is given credit for the discovery of the pion, Cesar Lattes is perhaps more responsible for its discovery. Powell was the research group head at the time and the tradition of the Nobel committe was to award the prize to the group leader. Cesar Lattes asked Kodak to include more boron in their emulsion plates making them more sensitive to mesons. Lattes also worked with Eugene Gardner to calcualte the pions mass.

Lattes exposed the plates on Mount Chacaltaya in the Bolivian Andes, near the capital La Paz and found ten two-meson decay events in which the secondary particle came to rest in the emulsion. The constant range of around 600 microns of the secondary meson in all cases led Lattes, Occhialini and Powell, in their October 1947 paper in 'Nature ', to postulate a two-body decay of the primary meson, which they called p or pion, to a secondary meson, m or muon, and one neutral particle. Subsequent mass measurements on twenty events gave the pion and muon masses as 260 and 205 times that of the electron respectively, while the lifetime of the pion was estimated to be some 10-8 s. Present-day values are 273.31 and 206.76 electron masses respectively and 2.6 x 10-8 s. The number of mesons coming to rest in the emulsion and causing a disintegration was found to be approximately equal to the number of pions decaying to muons. It was, therefore, postulated that the latter represented the decay of positively-charged pions and the former the nuclear capture of negatively-charged pions. Clearly the pions were the particles postulated by Yukawa.

In the cosmic ray emulsions they saw a negative pion (cosmic ray) get captured by a nucleus and a positive pion (cosmic ray) decay. The two pion types had similar tracks because of their similar masses.

## Nuclear Properties

NuclearProperties_Forest_NucPhys_I

The nucleus of an atom has such properties as spin, mangetic dipole and electric quadrupole moments. Nuclides also have stable and unstable states. Unstable nuclides are characterized by their decay mode and half lives.

### Decay Modes

Mode | Description |

Alpha decay | An alpha particle (A=4, Z=2) emitted from nucleus |

Proton emission | A proton ejected from nucleus |

Neutron emission | A neutron ejected from nucleus |

Double proton emission | Two protons ejected from nucleus simultaneously |

Spontaneous fission | Nucleus disintegrates into two or more smaller nuclei and other particles |

Cluster decay | Nucleus emits a specific type of smaller nucleus (A1, Z1) smaller than, or larger than, an alpha particle |

Beta-Negative decay | A nucleus emits an electron and an antineutrino |

Positron emission(a.k.a. Beta-Positive decay) | A nucleus emits a positron and a neutrino |

Electron capture | A nucleus captures an orbiting electron and emits a neutrino - The daughter nucleus is left in an excited and unstable state |

Double beta decay | A nucleus emits two electrons and two antineutrinos |

Double electron capture | A nucleus absorbs two orbital electrons and emits two neutrinos - The daughter nucleus is left in an excited and unstable state |

Electron capture with positron emission | A nucleus absorbs one orbital electron, emits one positron and two neutrinos |

Double positron emission | A nucleus emits two positrons and two neutrinos |

Gamma decay | Excited nucleus releases a high-energy photon (gamma ray) |

Internal conversion | Excited nucleus transfers energy to an orbital electron and it is ejected from the atom |

### Time

Time scales for nuclear related processes range from years to

seconds. In the case of radioactive decay the excited nucleus can take many years ( ) to decay (Half Life). Nuclear transitions which result in the emission of a gamma ray can take anywhere from to seconds.## Units and Dimensions

Variable | Definition |

1 fermi | m |

1 MeV | = | eV = J

1 a.m.u. | Atomic Mass Unit = 931.502 MeV |

## Resources

The following are resources available on the internet which may be useful for this class.

in particular

The Lund Nuclear Data Search Engine

Several Table of Nuclides

BNL

LANL

Korean Atomic Energy Research Institute

National Physical Lab (UK)

Table of Isotopes at Lawrence Berkeley National Laboratory

# Quantum Mechanics Review

Quantum_Mechanics_Review_Forest_NucPhys_I

# Nuclear Properties

NuclearProperties_Forest_NucPhys_I

# The Nuclear Force

# Nuclear Models

Given the basic elements of the nuclear potential from the last chapter, one may be tempted to construct the hamiltonian for a group of interacting nucleons in the form

where

- represent the kinetic energy of the ith nucleon
- represents the potential energy between two nucleons.

If you assume that the nuclear force is a two body force such that the force between any two nucleons doesn't change with the addition of more nucleons, Then you can solve the Schrodinger equation corresponding to the above Hamiltonian for A<5.

For A< 8 there is a technique called Green's function monte carlo which reportedly finds solution that are nearly exact. J. Carlson, Phys. Rev. C 36, 2026 - 2033 (1987), B. Pudliner, et. al., Phys. Rev. Lett. 74, 4396 - 4399 (1995)

## Shell Model

### Independent particle model

This part of the Shell model suggests that the properties of a nucleus with only one unpaired nucleon are determined by that one unpaired nucleon. The unpaired nucleon usually, though no necessarily, occupies the outer most shell as a valence nucleon.

### SN-130 Example

The low lying excited energy states for Sn-130 taken from the LBL website are given below.

File:Sn-130 LowLyingE Levels.tiff

The listing indicates that the ground state of Sn-130 is a spin 0 positive parity state. The first excited state of this nucleus is 1.22 MeV above the ground state and has . The next excited state is 1.95 MeV above the ground state and has .

Let's see how well the shell model does at predicting these

states## Liquid Drop Model

Bohr and Mottelson considered the nucleon in terms of its collective motion with vibrations and rotations that resembled a suspended drop of liquid.

## Electric Quadrupole Moment

Electric_QuadrupoleMoment_Forest_NuclPhys_I

# Nuclear Decay

Nuclear_Decay_Forest_NucPhys_I

# Nuclear Reactions

Forest_NucPhys_I_Nuclear_Reactions

# Electro Magnetic Interactions

# Weak Interactions

Neutrino

The min neutrino energy needed for this reaction assuming the electron energy is ignorable:

A reaction to the ground state of potassium is forbidden in this charged current electron neutrino reaction resulting in one or more gammas being emitted as the Potassium nucleus de-excited to the ground state. There are about 98 observed excited states of the K-40 nucleus.

Detecting this signal in DUNE means you need to see and electron and at least one gamma in coincidence.

Potassium 40 decay

89% of the time

10.72% of the time

0.001% of the time

Potassium has half life of

years.Potassium-Argon dating measures the amount of argon trapped in rock. Originally molten rock has no argon. After molten rock solidifies, the argon from decaying Potassium is trapped. In primordial material, Argon-39 is dominant. Argon-40 dominates in the earths atmosphere.

Argon-36,38,40 are stable.

Argon-39 is the longest lived isotope with a half life of 269 years

Argon-39 decay:

# Strong Interaction

# Applications

# Homework problems

# Midterm Exam Topics list

Basically everything before section 5.3 (The Nuclear Force). Section 5.3 and below is not included on the midterm.

Topics of emphasis:

- 1-D Schrodinger Equation based problems involving discrete potentials ( wells, steps) and continuous potentials (simple Harmonic, coulomb).
- Calculating form factors given the density of a nucleus
- Determining binding and nucleon mass separation energies
- , , and angular momentum operations
- Calculating scattering rates given the cross-section and a description of the experimental apparatus

Formulas given on test

Schrodinger Time independent 1-D equation

Particle Current Density

Form Factor

If the density has no

or dependenceCoulomb energy difference between point nucleus and one with uniform charge distribution

Nucleus Binding Energy

Neutron Separation energy

Proton Separation energy

Semiempirical Mass Formula

where

Parameter | Krane |

15.5 | |

16.8 | |

0.72 | |

23 | |

34 |

# Final

1.) Calculate the magnetic moment of a proton assuming that it may be described as a neutron with a positive pion

in an state.

2.) Show that the phase shift ( ) for the scattering of a neutron by a proton can be given by the equation

where

V = 36.7 MeV R = 2.1 fm

3.)

a.) Write the reaction equations for the following processes. Show all reaction products.

i.)

ii.)

iii.)

iv.)

b.) Determine the Q-values for the first two reactions above.

4.) Find the Quadrupole moment of using the shell model and compare to the experimental value of -0.37 barns.

5.) Find , using the shell model, for the following nuclei

a.)

b.)

c.)

d.)

6.) Use the shell model to predict the ground state spin and parity of the following nuclei:

a.)

b.)

c.)

d.)

7.) Tabulate the possible

states for a nucleus three quadrupole phonon state ( ). Show that the permitted resultant states are , , , , and .