Lesson 9 Gamma Ray Decay. Electromagnetic decay There are two types of electromagnetic decay,  -ray emission and internal conversion (IC). In both of.

Slides:



Advertisements
Similar presentations
The atom and its nucleus
Advertisements

Radioactive Decay. - Alpha Decay The emission of an particle from the nucleus of an atom is called alpha decay An alpha particle is just a helium nucleus.
Gamma Decay Readings: Modern Nuclear Chemistry, Chap. 9; Nuclear and Radiochemistry, Chapter 3 Energetics Decay Types Transition Probabilities Internal.
Isomer Spectroscopy in Near-Spherical Nuclei Lecture at the ‘School cum Workshop on Yrast and Near-Yrast Spectroscopy’ IIT Roorkee, October 2009 Paddy.
Gamma-ray strength functions Also called in the literature: radiative strength functions photon strength functions Presentation OCL group meeting Ann-Cecilie.
Gamma-Ray Spectra _ + The photomultiplier records the (UV) light emitted during electronic recombination in the scintillator. Therefore, the spectrum collected.
CHARACTERISTICS OF INTERACTIONS. In a radiation interaction, the radiation and the material with which it interacts may be considered as a single system.
Interactions of Radiation With Matter
H H H H H H 7- 1— H أجازة ( أجازة
PRACTICAL RADIATION PHYSICS FOR EMERGENCY MEDICAL PERSONNEL Module III.
X-radiation. X-rays are part of the electromagnetic spectrum. X-radiation (composed of X-rays) is a form of electromagnetic radiation. X- rays have a.
Light. Photons The photon is the gauge boson of the electromagnetic force. –Massless –Stable –Interacts with charged particles. Photon velocity depends.
When an nucleus releases the transition energy Q (say 14.4 keV) in a  -decay, the  does not carry the full 14.4 keV. Conservation of momentum requires.
NUCLEAR CHEMISTRY The Basics. The Nucleus The nucleus is composed of nucleons –protons –neutrons A nucleus is characterized by two numbers –atomic mass.
Chapter 30 Nuclear Physics
Happyphysics.com Physics Lecture Resources Prof. Mineesh Gulati Head-Physics Wing Happy Model Hr. Sec. School, Udhampur, J&K Website: happyphysics.com.
Alpha decay parent nucleus daughter nucleus Momentum conservation decides how the energy is distributed. r E 30 MeV 5 MeV.
Lesson 8 Beta Decay. Beta-decay Beta decay is a term used to describe three types of decay in which a nuclear neutron (proton) changes into a nuclear.
INTERACTION OF IONISING RADIATION WITH MATTER
Week 11 Lecture 27 Monday, Oct 30, 2006 NO CLASS : DPF06 conference Lecture 28 Wednesday, Nov 1, 2006 GammaDecaysGammaDecays Lecture 29 Friday, Nov 3,
Lesson 8 Beta Decay. Beta -decay Beta decay is a term used to describe three types of decay in which a nuclear neutron (proton) changes into a nuclear.
Lesson 7 Alpha Decay. Alpha decay (  ) Decay by the emission of doubly charged helium nuclei 4 He U  234 Th + 4 He  Z = -2,  N=-2,  A=-4.
P461 - decays III1 Gamma Decays If something (beta/alpha decay or a reaction) places a nucleus in an excited state, it drops to the lowest energy through.
Nuclear de-excitation Outline of approach… Source of radiation Propagation of radiation field Detection of radiation ?? nucleus.
Radioactivity – types of decays presentation for April 28, 2008 by Dr. Brian Davies, WIU Physics Dept.
Interactions with Matter
NUCLEAR STRUCTURE PHENOMENOLOGICAL MODELS
6-1 RFSS: Lecture 6 Gamma Decay Part 2 Readings: Modern Nuclear Chemistry, Chap. 9; Nuclear and Radiochemistry, Chapter 3 Energetics Decay Types Transition.
Radiology is concerned with the application of radiation to the human body for diagnostically and therapeutically purposes. This requires an understanding.
PHYS 580 Nuclear Structure Chapter5-Lecture1 GAMMA DECAY
6-1 RFSS: Lecture 6 Gamma Decay Part 1 Readings: Modern Nuclear Chemistry, Chap. 9; Nuclear and Radiochemistry, Chapter 3 Energetics Decay Types Transition.
Stopping Power The linear stopping power S for charged particles in a given absorber is simply defined as the differential energy loss for that particle.
NUCLEAR PHYSICS & RADIOACTIVITY PHYSICS - UNIT ONE.
Jag Tuli NSDD, Vienna, 4/2015 ENSDF Policies 4/15 Jagdish Tuli* National Nuclear Data Center Brookhaven National Laboratory * Brookhaven.
ENTC 4390 MEDICAL IMAGING RADIOACTIVE DECAY.
Mossbauer Spectroscopy
Nuclear Stability and Radioactivity AP Physics B Montwood High School R. Casao.
Structure of the Nucleus Every atom has a nucleus, a tiny but massive center.Every atom has a nucleus, a tiny but massive center. The nucleus is made up.
Properties of Light.
Lecture 1 Introduction to Nuclear Science. Composition of atoms Atoms are composed of electrons and nuclei. The electrons are held in the atom by a Coulomb.
Gamma Decay Energetics Decay Types Transition Probabilities
Chapter 10 Gamma Decay ● Introduction ◎ Energetics of γ Decay ● Decay Constant for γ Decay ◎ Classical Electromagnetic Radiation ● Quantum Description.
Nuclear Chemistry , Nuclear Chemistry The study of the properties and reactions of atomic nuclei Atoms with identical atomic numbers.
1 Alpha Decay  Because the binding energy of the alpha particle is so large (28.3 MeV), it is often energetically favorable for a heavy nucleus to emit.
PHYSICAL BACKGROUND ATOMIC STRUCTURE, NUCLEONS AND ACTIVITY
Medical Imaging Radiation I. Naked to the Bone: Medical Imaging in the Twentieth Century (Paperback)by Bettyann Kevles Bettyann Kevles E=mc2: A Biography.
Artificial Radioactivity
NUCLEAR CHEMISTRY Chapter 28. I. Introduction A. Nucleons 1. Neutrons and protons B. Nuclides 1. Atoms identified by the number of protons and neutrons.
NUCLEAR FORCES NOTES. Nuclear Forces Strong nuclear forces keep the nucleons together. These are powerful short-range force of attraction between the.
RFSS: Lecture 6 Gamma Decay
Basic Nuclear Physics - 2
Nuclear Chemistry. RadioactivityRadioactivity  The spontaneous decomposition of a nucleus to form a different nucleus accompanied by a release of energy.
Happyphysics.com Physics Lecture Resources Prof. Mineesh Gulati Head-Physics Wing Happy Model Hr. Sec. School, Udhampur, J&K Website: happyphysics.com.
Mineral Spectroscopy Visible Infrared Raman Mössbauer NMR.
Nuclear Decay. Radioactivity The emission of high-energy radiation or particles from the nucleus of a radioactive atom.
CHEM 312: Gamma Decay Readings: Modern Nuclear Chemistry, Chap. 9; Nuclear and Radiochemistry, Chapter 3 Energetics Decay Types Transition Probabilities.
Interaction of Radiation with Matter
 Nuclear Chemistry. Nuclear Vs. Chemical Reactions  Nuclear reactions involve a change in an atom’s nucleus, usually producing a different element.
W. Udo Schröder, 2005 Gamma Decay 1. W. Udo Schröder, 2005 Gamma Decay 2 Photons Photons: generated by moving charge distributions. Distributions can.
6-1 CHEM 312: Lecture 6 Gamma Decay Readings: Modern Nuclear Chemistry, Chap. 9; Nuclear and Radiochemistry, Chapter 3 Energetics Decay Types Transition.
Interactions of Ionizing Radiation
Mossbauer spectroscopy
Electromagnetic (gamma) decay
Determining Reduced Transition Probabilities for 152 ≤ A ≤ 248 Nuclei using Interacting Boson Approximation (IBA-1) Model By Dr. Sardool Singh Ghumman.
Review or Introduction to Atomic and Nuclear Physics
Introduction (Atomic and Nuclear Structure-Radioactivity)
PHL424: γ-decay γ-decay is an electromagnetic process where the nucleus decreases in excitation energy, but does not change proton or neutron numbers This.
CHEM 312: Lecture 6 Part 2 Gamma Decay
Three kinds of particle emission
Presentation transcript:

Lesson 9 Gamma Ray Decay

Electromagnetic decay There are two types of electromagnetic decay,  -ray emission and internal conversion (IC). In both of these decays  N=  Z=  A=0, with just a lowering of the excitation energy of the nucleus. In  -ray emission, most of the emitted energy appears in the form of a photon. These emitted photons are mono-energetic and have an energy corresponding to almost all of the energy difference between the final and initial state of the system. This is typically depicted as

Electromagnetic decay(cont.)  -rays are the most penetrating nuclear radiation and to attenuate them requires massive shielding. They represent an external radiation hazard. An example of a  -emitter is 60 Co. 60 Co is longer lived nuclide (t 1/2 =5.3 y) that emits  - particles, that populate the excited states of 60 Ni, which emits two  -rays of energy, 1.17 and 1.33 MeV. This nuclide can be created in an “Doomsday machine”, (Dr. Strangelove) with disastrous consequences. The second type of electromagnetic decay is internal conversion. In IC decay, the emitted energy is transferred (radiationlessly) to an orbital electron, ejecting that electron which carries away most of the decay energy.

Isomers, Isomeric Transitions Ordinary electromagnetic transitions take place within s. Occasionally one sees an electromagnetic transition with a lifetime of ns or greater. These transitions are called isomeric transitions (IT) and the originating states are called isomers.

Example of an IT

Energetics of Gamma Decay

Classification of Electromagnetic Decays The initial and final states have a definite angular momentum and parity. The photon carries away a definite amount of angular momentum. Angular momentum and parity must be conserved. Thus where the angular momentum carried away by the photon is

Classification of Electromagnetic Decays (cont.) Multipolarity is a measure of the angular momentum carried away by the photon.

Classification of Electromagnetic Decays (cont.) Transitions are classified as electric or magnetic based on whether the radiation is due to a shift in the charge distribution or a shift in the current distribution. Based upon the type of operator involved in the transition, there are restrictions on the parity change in the transition.

Classification of Electromagnetic Decays (cont.).

Example

Additional points No gamma ray transitions of type 0  0. Possible by IC Can get both electric and magnetic matrix elements contributing to a given decay probability Lowest multipolarity is most favored Electric matrix elements are generally greater than magnetic matrix elements of tthe same multipolarity. E2 and M1 transition rates are similar

Shell model estimates of electromagnetic transition rates Can model the electromagnetic transitions in the shell model as cuased by the change of a single nucleon from one shell model orbital to another. These estimates are referred to as the “Weisskopf single particle estimates” after Victor Weisskopf.

Shell model estimates of electromagnetic transition rates (cont.)

Weisskopf estimates are good within a factor of 10 usually. The Weisskopf estimate is used as unit to express gamma-ray transition rates, i.e., rates are expressed as the (measured rate/Weisskopf rate) or in terms of Weisskopf units (W.u.)

Gamma ray transition rates and the collective model The collective motion of a group of nucleons would be expected to produce a large disturbance in the electromagnetic field of a nucleus, leading to higher probability gamma ray transitions. This primarily affects E2 transition rates which are related to the nuclear quadrupole moment, which is large for deformed nuclei.

Gamma ray transition rates and the collective model(cont.) Within a rotational band

Gamma ray transition rates and the collective model(cont.) Odd A nuclei

Gamma ray transition rates and the collective model(cont.) K conservation Vibrational nuclei --enhanced 2+  2+ transitions

Internal conversion E IC =E transition -E electron binding energy

Internal conversion coefficients, 

Auger effect In internal conversion, create vacancy in electronic shell. This can be filled by an outer electron moving into the vacancy and emitting an X-ray. Sometimes the energy is not released in the form of an X-ray but transferred to another electron, causing it to be emitted, ie, sort of an “atomic internal conversion.” This is called the Auger effect.

Auger effect (cont.) The emitted electrons are called Auger electrons.

Auger effect (cont.) Probability of Auger emission fluorescence yield=fraction of vacancies filled by x-ray emission Auger yield=fraction of vacancies filled by Auger emission

Gamma Ray Angular Correlations The gamma rays emitted from a source are isotropic in direction. There is a way to see something other than isotropic emission and that is to observe two gamma rays that are emitted sequentially by a nucleus. The emission of the first gamma ray polarizes the nucleus, ie, establishes an orientation of the intermediate state.

Consider a 0  1  0 transition

Data Analysis

Mossbauer Effect Emission of a gamma ray causes the nucleus to recoil, with an energy E r =E  2 /2mc 2 Suppose we consider two nuclear states separated by an energy E 0. Then if we shine light on the lower state of energy E 0 + E r, then we can excite the higher state. When the higher state decays, it will emit a gamma ray of energy E 0 - E r, which will not excite another state. We can do two things to change this situation, ie, “clamp” the nuclei in a crystal, making m  m crystal and we can mechanically move one nucleus relative to another.

Voila! This is called recoilless resonant absorption or the Mossbauer effect.

So What? You have created an exquisitely sensitive “instrument”, that can respond to some very small changes, ~10 -6 eV. Use of the “instrument” 1.Measurement of G 2.Chemical studies of the environment of the nucleus

Mossbauer Nuclei