CHAPTER 33: PARTICLE PHYSICS

Similar documents
Lecture 14. Relic neutrinos Temperature at neutrino decoupling and today Effective degeneracy factor Neutrino mass limits Saha equation

Grand Canonical Ensemble

BETA DECAY VISUAL PHYSICS ONLINE

Pair (and Triplet) Production Effect:

Nuclear reactions The chain reaction

CHAPTER 4. The First Law of Thermodynamics for Control Volumes

Ερωτήσεις και ασκησεις Κεφ. 10 (για μόρια) ΠΑΡΑΔΟΣΗ 29/11/2016. (d)

Physics of Very High Frequency (VHF) Capacitively Coupled Plasma Discharges

The Hyperelastic material is examined in this section.

Chapter 8: Electron Configurations and Periodicity

ph People Grade Level: basic Duration: minutes Setting: classroom or field site

te Finance (4th Edition), July 2017.

Jones vector & matrices

fiziks Institute for NET/JRF, GATE, IIT JAM, M.Sc. Entrance, JEST, TIFR and GRE in Physics NUCLEAR AND PARTICLE PHYSICS NET/JRF (JUNE-2011)

Relate p and T at equilibrium between two phases. An open system where a new phase may form or a new component can be added

A=P=E M-A=N Alpha particle Beta Particle. Periodic table

Lecture 3: Phasor notation, Transfer Functions. Context

Physics 256: Lecture 2. Physics

Background: We have discussed the PIB, HO, and the energy of the RR model. In this chapter, the H-atom, and atomic orbitals.

Polytropic Process. A polytropic process is a quasiequilibrium process described by

Alpha and beta decay equation practice

Standard Model - Electroweak Interactions. Standard Model. Outline. Weak Neutral Interactions. Electroweak Theory. Experimental Tests.

Constituents of the Atom

Lucas Test is based on Euler s theorem which states that if n is any integer and a is coprime to n, then a φ(n) 1modn.

Classical Magnetic Dipole

ANALYSIS: The mass rate balance for the one-inlet, one-exit control volume at steady state is

Pion condensation with neutrinos

Hydrogen Atom and One Electron Ions

JEE-2017 : Advanced Paper 2 Answers and Explanations

Neutrinos. Overview. Pauli postulates Neutrino Discovery of neutrino flavours. Neutrino Interactions. Neutrino mass. Neutrino oscillations

Precision Standard Model Tests (at JLab)

Add sodium hydroxide solution

The following information relates to Questions 1 to 4:

Antonio Pich. IFIC, CSIC Univ. Valencia.

Contemporary, atomic, nuclear, and particle physics

The van der Waals interaction 1 D. E. Soper 2 University of Oregon 20 April 2012

September 23, Honors Chem Atomic structure.notebook. Atomic Structure

Analyzing Frequencies

Heisenberg Model. Sayed Mohammad Mahdi Sadrnezhaad. Supervisor: Prof. Abdollah Langari

Review - Probabilistic Classification

Determination of Vibrational and Electronic Parameters From an Electronic Spectrum of I 2 and a Birge-Sponer Plot

5.62 Physical Chemistry II Spring 2008

Math 34A. Final Review

Phy213: General Physics III 4/10/2008 Chapter 22 Worksheet 1. d = 0.1 m

1- Summary of Kinetic Theory of Gases

Phys 774: Nonlinear Spectroscopy: SHG and Raman Scattering

Economics 600: August, 2007 Dynamic Part: Problem Set 5. Problems on Differential Equations and Continuous Time Optimization

de/dx Effectively all charged particles except electrons

2. Laser physics - basics

Davisson Germer experiment Announcements:

Elements of Statistical Thermodynamics

PHYS ,Fall 05, Term Exam #1, Oct., 12, 2005

Consider a system of 2 simultaneous first order linear equations

Chapter 2: The Photosphere

0 +1e Radionuclides - can spontaneously emit particles and radiation which can be expressed by a nuclear equation.

Ch. 24 Molecular Reaction Dynamics 1. Collision Theory

The Fourier Transform

Higher order derivatives

Why is a E&M nature of light not sufficient to explain experiments?

ACOUSTIC WAVE EQUATION. Contents INTRODUCTION BULK MODULUS AND LAMÉ S PARAMETERS

Today. Wave-Matter Duality. Quantum Non-Locality. What is waving for matter waves?

orbiting electron turns out to be wrong even though it Unfortunately, the classical visualization of the

22/ Breakdown of the Born-Oppenheimer approximation. Selection rules for rotational-vibrational transitions. P, R branches.

NOTES FOR CHAPTER 17. THE BOLTZMANN FACTOR AND PARTITION FUNCTIONS. Equilibrium statistical mechanics (aka statistical thermodynamics) deals with the

A Note on Estimability in Linear Models

University of Illinois at Chicago Department of Physics. Thermodynamics & Statistical Mechanics Qualifying Examination

GPC From PeakSimple Data Acquisition

Electrochemistry L E O

Prod.C [A] t. rate = = =

Differentiation of Exponential Functions

September 27, Introduction to Ordinary Differential Equations. ME 501A Seminar in Engineering Analysis Page 1. Outline

Principles of Humidity Dalton s law

Neutrinos are chargeless, nearly massless particles Most abundant particle in the Universe Interact with matter via weak nuclear force

fiziks Institute for NET/JRF, GATE, IIT JAM, M.Sc. Entrance, JEST, TIFR and GRE in Physics Thermodynamics & Statistical Mechanics JEST-2012

Where k is either given or determined from the data and c is an arbitrary constant.

On the Hamiltonian of a Multi-Electron Atom

Chapter. 3 Wave & Particles I

PHYS-333: Problem set #2 Solutions

Precise Masses of particles

Linear Algebra. Definition The inverse of an n by n matrix A is an n by n matrix B where, Properties of Matrix Inverse. Minors and cofactors

(1) Then we could wave our hands over this and it would become:

Field Asymmetry and Thrust Control in the GDM Fusion Propulsion System

Properties of Quarks ( ) Isospin. π = 1, 1

Low-energy QED tests (and what we can learn from them)

Green Functions, the Generating Functional and Propagators in the Canonical Quantization Approach

Give the letter that represents an atom (6) (b) Atoms of A and D combine to form a compound containing covalent bonds.

Cosmology and particle physics

Exam 2 Thursday (7:30-9pm) It will cover material through HW 7, but no material that was on the 1 st exam.

Chemical Physics II. More Stat. Thermo Kinetics Protein Folding...

A central nucleus. Protons have a positive charge Electrons have a negative charge

High Energy Physics. Lecture 5 The Passage of Particles through Matter

26-Sep-16. Nuclear energy production. Nuclear energy production. Nuclear energy production. Nuclear energy production

Electrochemical Equilibrium Electromotive Force. Relation between chemical and electric driving forces

ME 200 Thermodynamics I Spring 2014 Examination 3 Thu 4/10/14 6:30 7:30 PM WTHR 200, CL50 224, PHY 112 LAST NAME FIRST NAME

Forces. Quantum ElectroDynamics. α = = We have now:

1997 AP Calculus AB: Section I, Part A

Collisions between electrons and ions

ECE507 - Plasma Physics and Applications

Pipe flow friction, small vs. big pipes

Supplementary Materials

Transcription:

Collg Physcs Studnt s Manual Chaptr 33 CHAPTER 33: PARTICLE PHYSICS 33. THE FOUR BASIC FORCES 4. (a) Fnd th rato of th strngths of th wak and lctromagntc forcs undr ordnary crcumstancs. (b) What dos that rato bcom undr crcumstancs n whch th forcs ar unfd? (a) From Tabl 33.1, w know that th rato of th wak forc to th lctromagntc 13 Wak 1 11 forc s 1. In othr words, th wak forc s 11 Elctromagntc 1 ordrs of magntud wakr than th lctromagntc forc. (b) Whn th forcs ar unfd, th da s that th four forcs ar just dffrnt manfstatons of th sam forc, so undr crcumstancs n whch th forcs ar unfd, th rato bcoms 1 to 1. (S Scton 33.6.) 33.3 ACCELERATORS CREATE MATTER FROM ENERGY 7. Suppos a W cratd n a bubbl chambr lvs for 5 5. 1 s. What dstanc dos t mov n ths tm f t s travlng at.9c? Snc ths dstanc s too short to mak a track, th prsnc of th W must b nfrrd from ts dcay products. Not that th tm s longr than th gvn W lftm, whch can b du to th statstcal natur of dcay or tm dlaton. Usng th dfnton of vlocty, w can dtrmn th dstanc travld by th W n a bubbl chambr: d vt 8 5 16 (.9)( 3. 1 m/s)( 5. 1 s) 1.35 1 m.135 fm 3

Collg Physcs Studnt s Manual Chaptr 33 33.4 PARTICLES, PATTERNS, AND CONSERVATION LAWS 13. Th s ts own antpartcl and dcays n th followng mannr: γ γ. What s th nrgy of ach γ ray f th s at rst whn t dcays? If th s at rst whn t dcays, ts total nrgy s just E mc. Snc ts ntal momntum s zro, ach γ ray wll hav qual but oppost momntum.. p p, so that p p, or p p. Snc a γ ray s a photon: E p c. f y1 y y1 y Thrfor, snc th momnta ar qual n magntud th nrgs of th γ rays ar qual: E 1 E. Thn, by consrvaton of nrgy, th ntal nrgy of th quals twc th nrgy of on of th γ rays: m c. Fnally, from Tabl 33., w can E dtrmn th rst mass nrgy of th, and th nrgy of ach γ ray s: m c E ( 135 MV c ) c 67.5 MV γ γ 19. (a) What s th uncrtanty n th nrgy rlasd n th dcay of a du to ts short lftm? (b) What fracton of th dcay nrgy s ths, notng that th dcay mod s γ γ (so that all th mass s dstroyd)? (a) Usng h Δ EΔt, w can calculat th uncrtanty n th nrgy, gvn th 4 lftm of th from Tabl 33.: h ΔE 4Δt 34 6.63 1 J s 6.8 1 17 4 (8.4 1 s) 19 1V J 1.6 1 19 3.9 V J (b) Th fracton of th dcay nrgy s dtrmnd by dvdng ths uncrtanty n th nrgy by th rst mass nrgy of th found n Tabl 33.: 33

Collg Physcs Studnt s Manual Chaptr 33 ΔE m 3.956 V 8.9 1 6 c ( 135. 1 V c ) c. 6 So th uncrtanty s approxmatly.9 1 prcnt of th rst mass nrgy. 33.5 QUARKS: IS THAT ALL THERE IS? 5. Rpat th prvous problm for th dcay mod Ω Λ K. (a) From Tabl 33.4, w know th quark composton of ach of th partcls nvolvd n ths dcay: Ω ( sss) Λ ( uds) K ( us). Thn, to dtrmn th chang n strangnss, w nd to subtract th ntal from th fnal strangnss, rmmbrng that a strang quark has a strangnss of - 1: ΔS S [ 1 ( 1) ] ( 3) 1 f S 1 1 1 (b) Usng Tabl 33.3, w know that B 1, 3 3 3 1 1 1 1 1 Bf 1, so th baryon numbr s ndd consrvd. Agan, 3 3 3 3 3 usng Tabl 33.3, th charg s: 1 1 1 1 1 1 Q q q, and Q q q q, so f 3 3 3 3 3 3 3 3 charg s ndd consrvd. Ths dcay dos not nvolv any lctrons or nutrnos, so all lpton numbrs ar zro bfor and aftr, and th lpton numbrs ar unaffctd by th dcay. (c) Usng Tabl 33.4, w can wrt th quaton n trms of ts consttunt quarks: ( us) or s u u d ( sss ) ( uds).snc thr s a chang n quark flavor, th wak nuclar forc s rsponsbl for th dcay.. (a) Is th dcay Σ n possbl consdrng th approprat consrvaton laws? Stat why or why not. (b) Wrt th dcay n trms of th quark consttunts of th 34

Collg Physcs Studnt s Manual Chaptr 33 partcls. (a) From Tabl 33.4, w know th quark composton of ach of th partcls nvolvd n th dcay: Σ ( dds) n( udd ) ( ud ). Th charg s consrvd at - 1. Th baryon numbr s consrvd at B1. All lpton numbrs ar consrvd at zro, and fnally th mass ntally s largr than th fnal mass: m > mn m ), so, ys, ths dcay s possbl by th consrvaton laws. ( Σ (b) Usng Tabl 33.4, w can wrt th quaton n trms of ts consttunt quarks: dds udd ud or s u u d 37. (a) How much nrgy would b rlasd f th proton dd dcay va th conjcturd racton p? (b) Gvn that th dcays to two γ s and that th fnd an lctron to annhlat, what total nrgy s ultmatly producd n proton dcay? (c) Why s ths nrgy gratr than th proton s total mass (convrtd to nrgy)? wll (a) Th nrgy rlasd from th racton s dtrmnd by th chang n th rst mass nrgs: ( ) ( ) ( ) ΔE mc Σ mc f m p m m c Usng Tabl 33., w can thn dtrmn ths dffrnc n rst mass nrgs: ( 938. 3 MV c 135. MV c. 511MV c ) c 8 8 MV 83 MV Δ E. (b) Th two γ rays wll carry a total nrgy of th rst mass nrgy of th : γ ΔE m c 135. MV Th postron/lctron annhlaton wll gv off th rst mass nrgs of th postron and th lctron: γ ΔE m c (.511MV) 1. MV So, th total nrgy would b th sum of all ths nrgs: E ΔE ΔE Δ 938.8 MV Δ tot E 35

Collg Physcs Studnt s Manual Chaptr 33 (c) Bcaus th total nrgy ncluds th annhlaton nrgy of an xtra lctron. So th full racton should b ( p ) 4γ. 33.6 GUTS: THE UNIFICATION OF FORCES 43. Intgratd Concpts Th ntnsty of cosmc ray radaton dcrass rapdly wth ncrasng nrgy, but thr ar occasonally xtrmly nrgtc cosmc rays that crat a showr of radaton from all th partcls thy crat by strkng a nuclus n th atmosphr as sn n th fgur gvn blow. Suppos a cosmc ray partcl havng an nrgy of avragng 1 1 GV convrts ts nrgy nto partcls wth masss MV/ c. (a) How many partcls ar cratd? (b) If th partcls ran down on a 1. - km ara, how many partcls ar thr pr squar mtr? (a) To dtrmn th numbr of partcls cratd, dvd th cosmc ray partcl nrgy by th avrag nrgy of ach partcl cratd: 1 cosmc ray nrgy 1 GV # of partcls cratd 5 1 nrgy partcl cratd c (. GV c ) 1 (b) Dvd th numbr of partcls by th ara thy ht: 5 1 partcls 1 partcls m 5 ( 1 m) 1 4 partcls m 49. Intgratd Concpts Suppos you ar dsgnng a proton dcay xprmnt and you can dtct 5 prcnt of th proton dcays n a tank of watr. (a) How many klograms of watr would you nd to s on dcay pr month, assumng a lftm of 1 y? (b) How many cubc mtrs of watr s ths? (c) If th actual lftm s 1 33 y, how long would you hav to wat on an avrag to s a sngl proton dcay? (a) On avrag, on proton dcays vry 1 y 1 1 months. So for on dcay vry month, you would nd: 36

Collg Physcs Studnt s Manual Chaptr 33 1dcay N 1 1 1 1 months/dcay N month 1 protons Snc you dtct only 5% of th actual dcays, you nd twc ths numbr of protons to obsrv on dcay pr month, or know that on N 4 1 protons. Now, w H O molcul has 1 protons (1 from ach hydrogn plus 8 from 3 th oxygn), so w nd 4 1 H O. Fnally, snc w know how many molculs w nd, and w know th molar mass of watr, w can dtrmn th numbr of klograms of watr w nd. 3 1mol. 18 kg 5 ( 4 1 molculs ) 7. 1 kg of watr 6. 1 (b) Now, w know th dnsty of watr, 3 molculs mol 3 ρ 1 kg/m, so w can dtrmn th 3 1m V mρ 7. 1 kg 7. 1 m 1 kg 5 3 volum of watr w nd: ( ) 3 (c) If w had 7. 1 m of watr, and th actual dcay rat was 1 33 y, rathr than 1 y, a dcay would occur 1 tms lss oftn, and w would hav to wat on avrag 1 months to s a dcay. 37