From Classical to Quantum mechanics

Size: px
Start display at page:

Download "From Classical to Quantum mechanics"

Transcription

1 From Classical to Quantum mcanics Engl & Rid vrij Univrsitit amstrdam Classical wav baviour Ligt is a wav Two-slit xprimnt wit potons (81-85) 1

2 On sourc Intrfrnc sourcs ttp:// ttp:// On narrow slit On wid slit ttp:// ttp:// narrow slits Two-slit xprimnt wit ligt ttp://

3 Non-classical baviour of ligt Non-classical baviour of ligt Two-slit xprimnt wit potons (81-85) Blac body radiation (77-78) Hot Stl and Pyromtr Spctral nrgy dnsity de/df Enrgy dnsity low tmpratur deω ω 3 π c P5.67 x 10-8 T 4 [W/m ] 300 K 600 K 900 K 100 K ω ω B T Poton nrgy [V] 1 V nrgy is Hz T nrgy of potons is quantizd E f ω deω ω π c 3 ω ω B T 1 Y Axis Titl Bacground blacbody radiation deω ω π c 3 ω ω B T 1 T.76 K X Axis Titl ttp:// 3

4 K variations Non-classical baviour of ligt Two-slit xprimnt wit potons (81-85) Blac body radiation (77-78) Potolctric ffct (79-80) Gorg F. Smoot Jon C. Matr Potolctric ffct 1 Potolctric ffct 0 0 Potolctric ffct 3 Potolctric ffct 4 0 Wa ngativ voltag 0 4

5 Potolctric ffct 5 Exprimntal rsults _ Larg ngativ voltag 0 + Stopping potntial (V) Potassium Tungstn Potassium Tungstn / / x x x10 15 Frquncy of ligt (s -1 ) Non-classical baviour of ligt X-rays Two-slit xprimnt wit potons (81-85) Blac body radiation (77-78) Potolctric ffct (79-80) X-ray production _ + Willm Rontgn s laboratory Willm Rontgn potograps ttp:// ttp:// 5

6 Modrn X-ray tub X-ray spctra Targt Bryllium window Focus cup Tungstn filamnt Intnsity Poton nrgy (V) Non-classical baviour of ligt T positiv lctron Two-slit xprimnt wit potons (81-85) Blac body radiation (77-78) Potolctric ffct (79-80) X-ray production Pair production Pair cration discovry Bubbl cambr 6

7 Pair cration simulation Pair production nuclus positron poton lctron Non-classical baviour of ligt Compton s papr Two-slit xprimnt wit potons (81-85) Blac body radiation (77-78) Potolctric ffct (79-80) X-ray production Pair production Compton ffct Compton ffct Assumption: poton as momntum /λ y λ λ cos m c Θ x ϕ ( 1 Θ) cos Θ + γmu cosϕ ' λ λ sin Θ γmu sin ϕ ' λ λ c c + mc + γmc ' λ λ y λ λ cos m c Θ x ϕ ( 1 Θ) 7

8 Non-classical baviour of ligt Two-slit xprimnt wit on poton at a tim Two-slit xprimnt wit potons (81-85) Blac body radiation (77-78) Potolctric ffct (79-80) X-ray production Pair production Compton ffct Two-slit xprimnt wit on poton (81-85) Non-classical baviour of ligt Conclusions for ligt Two-slit xprimnt wit potons (81-85) Blac body radiation (77-78) Potolctric ffct (79-80) X-ray production Pair production Compton ffct Two-slit xprimnt wit on poton (81-85) E f ω E f ω E f ω E f ω p mv λ Singl poton as still a wav caractr Dpnding on t typ of xprimnt ligt can b dscribd as a wav or as particls T ligt particls ar potons. T nrgy of a poton wit an angular frquncy ω is T momntum of a poton wit wav vctor is E ω p Non-classical baviour of particls Non-classical baviour of particls Two-slit xprimnt wit lctrons (81-85) Davisson and Grmr xprimnt (81) Elctron microscop (lctur) Nutron diffraction (lctur) 8

9 Non-classical baviour of particls Two-slit xprimnt for lctrons Two-slit xprimnt wit lctrons (81-85) Two-slit : quantitativ analysis Two-slit : intrfrnc Amplitud Two-slit : dstructiv intrfrnc Two-slit : constructiv intrfrnc 9

10 Elctrons+potons Non-classical baviour of particls Ψ n lctrons Two-slit xprimnt wit lctrons (81-85) Davisson and Grmr xprimnt (81) potons Davisson original papr Dtail of t original papr Davisson-Grmr xprimnt Exprimntal rsults θ d 10

11 Davisson-Grmr xprimnt Davisson-Grmr xprimnt 3 X θ θ d d Elctron scattring at t surfac Non-classical baviour of particls θ Two-slit xprimnt wit lctrons (81-85) Davisson and Grmr xprimnt (81) Elctron microscop (lctur) d d sinθ nλ Scanning lctron microscop Non-classical baviour of particls λ mv Two-slit xprimnt wit lctrons (81-85) Davisson and Grmr xprimnt (81) Elctron microscop (lctur) Nutron diffraction (lctur) 11

12 Elctron scattring in t bul Nutron diffraction θ Nutrons av also a wav caractr D D cosθ nλ Conclusions for particls Two-slit xprimnt wit lctrons (81-85) Davisson and Grmr xprimnt (81) Elctron microscop (lctur) Nutron diffraction (lctur) ω E p Gussing Scrödingr s quation for a fr particl Wav-particl duality Wat av w larnd so far? From wav to particl From particl to wav Scrödingr quation p mv λ E ν ω On would also li to av 1 p E m vparticl m ω m λ p E ν p E ω ( ) 1 p ω E m vparticl m m 1

13 Wat ar w looing for? A wav so tat: T intnsity of t wav is proportional to t dnsity of particls ω m Ψ n Tis wav sould b solution of a wav quation u t u x V u u α β t x ω V αω β ω m Nota bn: tis is only possibl wit a complx wav i(x-ωt). It dos not wor wit sin or cosin functions How to coos α and β? Insrt i(x-ωt) into α ( i) β m u u i m x t u u α β t x ( ) α( ω) β( )( ) β ix ωt ix ( ωt) ix ( ωt) i i i ω m Ψ Ψ i m x t Hisnbrg s uncrtainty principl As i(x-ωt) is a complx wav w cannot simply ta t squar, but Ψ n Ψ ( x, t) Fr particl wav function i A ( x ωt ) is a solution of Scrödingr s quation Ψ Ψ i m x t ( x ωt ) i( x ωt ) i Ψ( x, t) A A A Many i ( x ) ωt ar ncssary to localiz a wav function x x 1 Ψ constant Tis is not ralistic for a particl 13

14 Hisnbrg s Uncrtainty Principl Hisnbrg s Uncrtainty Principl x 1 ( ) x p x x p x E x t 3 tims quantum pysics Elctron tunnling p x Hisnbrg s uncrtainty principl Spin of t lctron Atoms cannot b vanisingly small Many i ( x ) ωt ar ncssary to localiz a wav function V g d ω m Vg d m p mv v m m particl T vlocity of a particl is givn by t group vlocity V g d ω m Vg d m p mv v m m particl 14

15 T group vlocity is compltly diffrnt from t pas vlocity V pas ω ω m ω Vpas m p mv v m m particl V g d ω m Vg d m p mv v m m particl Gussing Scrödingr s quation for a particl in a potntial Potntial nrgy Total nrgy F E total E intic + U x v ½mv +½Kx x x Forc F-Kx U ½Kx F U ½Kx Wor ÛFdx - Potntial nrgy U x x How to introduc potntial nrgy? Stationary stats Insrt i(x-ωt) into Ψ Ψ i m x t givs W loo for solutions of t tim-dpndnt Scrödingr quation Kintic nrgy m ω Kintic + nrgy Total nrgy in t form Ψ Ψ + U( x)ψ i m x t Ψ ( x, t) Φ( x) Et i and find m U x + ( ) ω Ψ Ψ + U( x)ψ i m x t Φ + U( x) Φ EΦ m x Tis is t tim-indpndnt Scrödingr quation for stationary stats (standing wavs) 15

Physics 43 HW #9 Chapter 40 Key

Physics 43 HW #9 Chapter 40 Key Pysics 43 HW #9 Captr 4 Ky Captr 4 1 Aftr many ours of dilignt rsarc, you obtain t following data on t potolctric ffct for a crtain matrial: Wavlngt of Ligt (nm) Stopping Potntial (V) 36 3 4 14 31 a) Plot

More information

Chapter. 3 Wave & Particles I

Chapter. 3 Wave & Particles I Announcmnt Cours wbpag http://highnrgy.phys.ttu.du/~sl/2402/ Txtbook PHYS-2402 Lctur 8 Quiz 1 Class avrag: 14.2 (out of 20) ~ 70% Fb. 10, 2015 HW2 (du 2/19) 13, 17, 23, 25, 28, 31, 37, 38, 41, 44 Chaptr.

More information

Davisson Germer experiment Announcements:

Davisson Germer experiment Announcements: Davisson Grmr xprimnt Announcmnts: Homwork st 7 is du Wdnsday. Problm solving sssions M3-5, T3-5. Th 2 nd midtrm will b April 7 in MUEN E0046 at 7:30pm. BFFs: Davisson and Grmr. Today w will go ovr th

More information

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

Why is a E&M nature of light not sufficient to explain experiments? 1 Th wird world of photons Why is a E&M natur of light not sufficint to xplain xprimnts? Do photons xist? Som quantum proprtis of photons 2 Black body radiation Stfan s law: Enrgy/ ara/ tim = Win s displacmnt

More information

Atomic Physics. Final Mon. May 12, 12:25-2:25, Ingraham B10 Get prepared for the Final!

Atomic Physics. Final Mon. May 12, 12:25-2:25, Ingraham B10 Get prepared for the Final! # SCORES 50 40 30 0 10 MTE 3 Rsults P08 Exam 3 0 30 40 50 60 70 80 90 100 SCORE Avrag 79.75/100 std 1.30/100 A 19.9% AB 0.8% B 6.3% BC 17.4% C 13.1% D.1% F 0.4% Final Mon. Ma 1, 1:5-:5, Ingraam B10 Gt

More information

Final exam: Tuesday, May 11, 7:30-9:30am, Coates 143

Final exam: Tuesday, May 11, 7:30-9:30am, Coates 143 Final exam: Tuesday, May 11, 7:30-9:30am, Coates 143 Approximately 7 questions/6 problems Approximately 50% material since last test, 50% everyting covered on Exams I-III About 50% of everyting closely

More information

Atomic energy levels. Announcements:

Atomic energy levels. Announcements: Atomic nrgy lvls Announcmnts: Exam solutions ar postd. Problm solving sssions ar M3-5 and Tusday 1-3 in G-140. Will nd arly and hand back your Midtrm Exam at nd of class. http://www.colorado.du/physics/phys2170/

More information

Chapter 1 Late 1800 s Several failures of classical (Newtonian) physics discovered

Chapter 1 Late 1800 s Several failures of classical (Newtonian) physics discovered Chaptr 1 Lat 1800 s Svral failurs of classical (Nwtonian) physics discovrd 1905 195 Dvlopmnt of QM rsolvd discrpancis btwn xpt. and classical thory QM Essntial for undrstanding many phnomna in Chmistry,

More information

General Physics (PHY 2140)

General Physics (PHY 2140) Gnral Pysics (PHY 140) Lctur 16 Modrn Pysics Last lctur: 1. Quantum pysics Wav function Uncrtainty rlations Ligtning Rviw ΔΔ x p π ΔEΔt π Atomic Pysics Early modls of t atom Atomic spctra Bor s tory of

More information

Davisson Germer experiment

Davisson Germer experiment Announcmnts: Davisson Grmr xprimnt Homwork st 5 is today. Homwork st 6 will b postd latr today. Mad a good guss about th Nobl Priz for 2013 Clinton Davisson and Lstr Grmr. Davisson won Nobl Priz in 1937.

More information

PH300 Modern Physics SP11 Final Essay. Up Next: Periodic Table Molecular Bonding

PH300 Modern Physics SP11 Final Essay. Up Next: Periodic Table Molecular Bonding PH Modrn Physics SP11 Final Essay Thr will b an ssay portion on th xam, but you don t nd to answr thos qustions if you submit a final ssay by th day of th final: Sat. 5/7 It dosnʼt mattr how smart you

More information

Introduction to the quantum theory of matter and Schrödinger s equation

Introduction to the quantum theory of matter and Schrödinger s equation Introduction to th quantum thory of mattr and Schrödingr s quation Th quantum thory of mattr assums that mattr has two naturs: a particl natur and a wa natur. Th particl natur is dscribd by classical physics

More information

Compton Scattering. There are three related processes. Thomson scattering (classical) Rayleigh scattering (coherent)

Compton Scattering. There are three related processes. Thomson scattering (classical) Rayleigh scattering (coherent) Comton Scattring Tr ar tr rlatd rocsss Tomson scattring (classical) Poton-lctron Comton scattring (QED) Poton-lctron Raylig scattring (cornt) Poton-atom Tomson and Raylig scattring ar lasticonly t dirction

More information

Quantum transport in 2D

Quantum transport in 2D Quantum transport in D Quantum transport : wat is conductanc? mtallic ring atomic contact nanotub Landaur-üttikr formalism of quantum transport D gas grapn wir ntwork GRAPHENE & CO, Cargès April -3, 08

More information

Hydrogen Atom and One Electron Ions

Hydrogen Atom and One Electron Ions Hydrogn Atom and On Elctron Ions Th Schrödingr quation for this two-body problm starts out th sam as th gnral two-body Schrödingr quation. First w sparat out th motion of th cntr of mass. Th intrnal potntial

More information

Characteristics of Gliding Arc Discharge Plasma

Characteristics of Gliding Arc Discharge Plasma Caractristics of Gliding Arc Discarg Plasma Lin Li( ), Wu Bin(, Yang Ci(, Wu Cngkang ( Institut of Mcanics, Cins Acadmy of Scincs, Bijing 8, Cina E-mail: linli@imc.ac.cn Abstract A gliding arc discarg

More information

Physics 2D Lecture Slides Lecture 12: Jan 28 th 2004

Physics 2D Lecture Slides Lecture 12: Jan 28 th 2004 Brian Wcht, th TA, is away this wk. I will substitut for his offic hours (in my offic 3314 Mayr Hall, discussion and PS sssion. Pl. giv all rgrad rqusts to m this wk (only) Quiz 3 Will Covr Sctions.1-.5

More information

Lecture 28 Title: Diatomic Molecule : Vibrational and Rotational spectra

Lecture 28 Title: Diatomic Molecule : Vibrational and Rotational spectra Lctur 8 Titl: Diatomic Molcul : Vibrational and otational spctra Pag- In this lctur w will undrstand th molcular vibrational and rotational spctra of diatomic molcul W will start with th Hamiltonian for

More information

Phys 402: Nonlinear Spectroscopy: SHG and Raman Scattering

Phys 402: Nonlinear Spectroscopy: SHG and Raman Scattering Rquirmnts: Polariation of Elctromagntic Wavs Phys : Nonlinar Spctroscopy: SHG and Scattring Gnral considration of polariation How Polarirs work Rprsntation of Polariation: Jons Formalism Polariation of

More information

Contemporary, atomic, nuclear, and particle physics

Contemporary, atomic, nuclear, and particle physics Contmporary, atomic, nuclar, and particl physics 1 Blackbody radiation as a thrmal quilibrium condition (in vacuum this is th only hat loss) Exampl-1 black plan surfac at a constant high tmpratur T h is

More information

Dual Nature of Matter and Radiation

Dual Nature of Matter and Radiation Higr Ordr Tinking Skill Qustions Dual Natur of Mattr and Radiation 1. Two bas on of rd ligt and otr of blu ligt of t sa intnsity ar incidnt on a tallic surfac to it otolctrons wic on of t two bas its lctrons

More information

ELEMENTARY QUANTUM MECHANICS

ELEMENTARY QUANTUM MECHANICS Pag 1 of 9 ELEMENTARY QUANTUM MECHANICS 1. INTRODUCTION Th triumph of modrn physics is th triumph of quantum physics. Quantum physics (mchanics) Grw out of failurs of classical physics Launchd by xprimnts

More information

Quantum Physics ANSWERS TO QUESTIONS CHAPTER OUTLINE

Quantum Physics ANSWERS TO QUESTIONS CHAPTER OUTLINE CHAPTER OUTNE 8 Blackbody Radiation and Planck s Tory 8 T Potolctric Effct 83 T Compton Effct 84 Potons and Elctromagntic Wavs 85 T Wav Proprtis of Particls 86 T Quantum Particl 87 T Doubl-Slit Eprimnt

More information

APP-IV Introduction to Astro-Particle Physics. Maarten de Jong

APP-IV Introduction to Astro-Particle Physics. Maarten de Jong APP-IV Introduction to Astro-Particl Physics Maartn d Jong 1 cosmology in a nut shll Hubbl s law cosmic microwav background radiation abundancs of light lmnts (H, H, ) Hubbl s law (199) 1000 vlocity [km/s]

More information

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

Background: We have discussed the PIB, HO, and the energy of the RR model. In this chapter, the H-atom, and atomic orbitals. Chaptr 7 Th Hydrogn Atom Background: W hav discussd th PIB HO and th nrgy of th RR modl. In this chaptr th H-atom and atomic orbitals. * A singl particl moving undr a cntral forc adoptd from Scott Kirby

More information

Physics 2D Lecture Slides Lecture 14: Feb 1 st 2005

Physics 2D Lecture Slides Lecture 14: Feb 1 st 2005 Physics D Lctur Slids Lctur 14: Fb 1 st 005 Vivk Sharma UCSD Physics Compton Effct: what should Happn Classically? Plan wav [f,λ] incidnt on a surfac with loosly bound lctrons intraction of E fild of EM

More information

Lecture 37 (Schrödinger Equation) Physics Spring 2018 Douglas Fields

Lecture 37 (Schrödinger Equation) Physics Spring 2018 Douglas Fields Lctur 37 (Schrödingr Equation) Physics 6-01 Spring 018 Douglas Filds Rducd Mass OK, so th Bohr modl of th atom givs nrgy lvls: E n 1 k m n 4 But, this has on problm it was dvlopd assuming th acclration

More information

4E : The Quantum Universe. Lecture 5, April 5 Vivek Sharma

4E : The Quantum Universe. Lecture 5, April 5 Vivek Sharma 4E : Th Quantum Univrs Lctur 5, April 5 Vivk Sharma modphys@hpmail.ucsd.du An X-ray Tub from 0 th Cntury Xray Th High Enrgy Acclrator of 1900s: producd nrgtic light : X Ray, gav nw optic to subatomic world

More information

6. The Interaction of Light and Matter

6. The Interaction of Light and Matter 6. Th Intraction of Light and Mattr - Th intraction of light and mattr is what maks lif intrsting. - Light causs mattr to vibrat. Mattr in turn mits light, which intrfrs with th original light. - Excitd

More information

2. Background Material

2. Background Material S. Blair Sptmbr 3, 003 4. Background Matrial Th rst of this cours dals with th gnration, modulation, propagation, and ction of optical radiation. As such, bic background in lctromagntics and optics nds

More information

The pn junction: 2 Current vs Voltage (IV) characteristics

The pn junction: 2 Current vs Voltage (IV) characteristics Th pn junction: Currnt vs Voltag (V) charactristics Considr a pn junction in quilibrium with no applid xtrnal voltag: o th V E F E F V p-typ Dpltion rgion n-typ Elctron movmnt across th junction: 1. n

More information

Physics 2D Lecture Slides. Oct 21. UCSD Physics. Vivek Sharma

Physics 2D Lecture Slides. Oct 21. UCSD Physics. Vivek Sharma Physics D Lctur Slids Oct 1 Vivk Sharma UCSD Physics Modrn Viw of Photolctric Effct E = hf = KE+ ϕ Is h sam in Photolctric Effct as in BBQ Radiation? Slop h = 6.66 x 10-34 JS Einstin Nobl Priz! No mattr

More information

38. Photons and Matter Waves

38. Photons and Matter Waves 38. Potons and Matter Waves Termal Radiation and Black-Body Radiation Color of a Tungsten filament as temperature increases Black Red Yellow Wite T Termal radiation : Te radiation depends on te temperature

More information

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

High Energy Physics. Lecture 5 The Passage of Particles through Matter High Enrgy Physics Lctur 5 Th Passag of Particls through Mattr 1 Introduction In prvious lcturs w hav sn xampls of tracks lft by chargd particls in passing through mattr. Such tracks provid som of th most

More information

HYSTERESIS AND BLEACHING OF ABSORPTION BY ELECTRONS ON HELIUM

HYSTERESIS AND BLEACHING OF ABSORPTION BY ELECTRONS ON HELIUM HYSERESIS AND BLEACHING O ABSORPION BY ELECRONS ON HELIUM D. Ryvkin, 1 M.J. La, and M.I. Dykman 1 1 Dpartmnt of Physics and Astronomy, Michigan Stat Univrsity Royal Holloway, Univrsity of London Dynamics

More information

PHYSICS 489/1489 LECTURE 7: QUANTUM ELECTRODYNAMICS

PHYSICS 489/1489 LECTURE 7: QUANTUM ELECTRODYNAMICS PHYSICS 489/489 LECTURE 7: QUANTUM ELECTRODYNAMICS REMINDER Problm st du today 700 in Box F TODAY: W invstigatd th Dirac quation it dscribs a rlativistic spin /2 particl implis th xistnc of antiparticl

More information

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

orbiting electron turns out to be wrong even though it Unfortunately, the classical visualization of the Lctur 22-1 Byond Bohr Modl Unfortunatly, th classical visualization of th orbiting lctron turns out to b wrong vn though it still givs us a simpl way to think of th atom. Quantum Mchanics is ndd to truly

More information

Studies of Turbulence and Transport in Alcator C-Mod Ohmic Plasmas with Phase Contrast Imaging and Comparisons with GYRO*

Studies of Turbulence and Transport in Alcator C-Mod Ohmic Plasmas with Phase Contrast Imaging and Comparisons with GYRO* Studis of Turbulnc and Transport in Ohmic Plasmas with Phas Contrast Imaging and Comparisons with GYRO* L. Lin 1, M. Porkolab 1, E.M. Edlund 1, J.C. Rost 1, M. Grnwald 1, D.R. Mikklsn 2, N. Tsujii 1 1

More information

The failure of the classical mechanics

The failure of the classical mechanics h failur of th classical mchanics W rviw som xprimntal vidncs showing that svral concpts of classical mchanics cannot b applid. - h blac-body radiation. - Atomic and molcular spctra. - h particl-li charactr

More information

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

Today. Wave-Matter Duality. Quantum Non-Locality. What is waving for matter waves? Today Wav-Mattr Duality HW 7 and Exam 2 du Thurs. 8pm 0 min rcap from last lctur on QM Finish QM odds and nds from ch.4 Th Standard Modl 4 forcs of Natur Fundamntal particls of Natur Fynman diagrams EM

More information

(most) due to long range e m forces i.e. via atomic collisions or due to short range nuclear collisions or through decay ( = weak interactions)

(most) due to long range e m forces i.e. via atomic collisions or due to short range nuclear collisions or through decay ( = weak interactions) Spring 01, P67, YK Monday January 30, 01 8 Obsrvabl particl dtction ffcts ar : (most) du to long rang m forcs i.. via atomic collisions or du to short rang nuclar collisions or through dcay ( = wak intractions)

More information

Ch. 24 Molecular Reaction Dynamics 1. Collision Theory

Ch. 24 Molecular Reaction Dynamics 1. Collision Theory Ch. 4 Molcular Raction Dynamics 1. Collision Thory Lctur 16. Diffusion-Controlld Raction 3. Th Matrial Balanc Equation 4. Transition Stat Thory: Th Eyring Equation 5. Transition Stat Thory: Thrmodynamic

More information

Quasi-Classical States of the Simple Harmonic Oscillator

Quasi-Classical States of the Simple Harmonic Oscillator Quasi-Classical Stats of th Simpl Harmonic Oscillator (Draft Vrsion) Introduction: Why Look for Eignstats of th Annihilation Oprator? Excpt for th ground stat, th corrspondnc btwn th quantum nrgy ignstats

More information

Schrodinger Equation in 3-d

Schrodinger Equation in 3-d Schrodingr Equation in 3-d ψ( xyz,, ) ψ( xyz,, ) ψ( xyz,, ) + + + Vxyz (,, ) ψ( xyz,, ) = Eψ( xyz,, ) m x y z p p p x y + + z m m m + V = E p m + V = E E + k V = E Infinit Wll in 3-d V = x > L, y > L,

More information

Title: Vibrational structure of electronic transition

Title: Vibrational structure of electronic transition Titl: Vibrational structur of lctronic transition Pag- Th band spctrum sn in th Ultra-Violt (UV) and visibl (VIS) rgions of th lctromagntic spctrum can not intrprtd as vibrational and rotational spctrum

More information

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

22/ Breakdown of the Born-Oppenheimer approximation. Selection rules for rotational-vibrational transitions. P, R branches. Subjct Chmistry Papr No and Titl Modul No and Titl Modul Tag 8/ Physical Spctroscopy / Brakdown of th Born-Oppnhimr approximation. Slction ruls for rotational-vibrational transitions. P, R branchs. CHE_P8_M

More information

de/dx Effectively all charged particles except electrons

de/dx Effectively all charged particles except electrons de/dx Lt s nxt turn our attntion to how chargd particls los nrgy in mattr To start with w ll considr only havy chargd particls lik muons, pions, protons, alphas, havy ions, Effctivly all chargd particls

More information

Intro to Nuclear and Particle Physics (5110)

Intro to Nuclear and Particle Physics (5110) Intro to Nuclar and Particl Physics (5110) March 09, 009 Frmi s Thory of Bta Dcay (continud) Parity Violation, Nutrino Mass 3/9/009 1 Final Stat Phas Spac (Rviw) Th Final Stat lctron and nutrino wav functions

More information

ATOMIC PHYSICS PREVIOUS EAMCET QUESTIONS ENGINEERING

ATOMIC PHYSICS PREVIOUS EAMCET QUESTIONS ENGINEERING ATOMIC PHYSICS PREVIOUS EAMCET QUESTIONS ENGINEERING 9. Te work function of a certain metal is. J. Ten te maximum kinetic energy of potoelectrons emitted by incident radiation of wavelengt 5 A is: (9 E)

More information

CHAPTER 5 Wave Properties of Matter and Quantum Mechanics I

CHAPTER 5 Wave Properties of Matter and Quantum Mechanics I CHAPTER 5 Wave Properties of Matter and Quantum Mechanics I 5.1 X-Ray Scattering 5.2 De Broglie Waves 5.3 Electron Scattering 5.4 Wave Motion 5.5 Waves or Particles? 5.6 Uncertainty Principle 5.7 Probability,

More information

Pair (and Triplet) Production Effect:

Pair (and Triplet) Production Effect: Pair (and riplt Production Effct: In both Pair and riplt production, a positron (anti-lctron and an lctron (or ngatron ar producd spontanously as a photon intracts with a strong lctric fild from ithr a

More information

ECE507 - Plasma Physics and Applications

ECE507 - Plasma Physics and Applications ECE507 - Plasma Physics and Applications Lctur 7 Prof. Jorg Rocca and Dr. Frnando Tomasl Dpartmnt of Elctrical and Computr Enginring Collisional and radiativ procsss All particls in a plasma intract with

More information

REGISTER!!! The Farmer and the Seeds (a parable of scientific reasoning) Class Updates. The Farmer and the Seeds. The Farmer and the Seeds

REGISTER!!! The Farmer and the Seeds (a parable of scientific reasoning) Class Updates. The Farmer and the Seeds. The Farmer and the Seeds How dos light intract with mattr? And what dos (this say about) mattr? REGISTER!!! If Schrödingr s Cat walks into a forst, and no on is around to obsrv it, is h rally in th forst? sourc unknown Phys 1010

More information

UNIT-1 MODERN PHYSICS

UNIT-1 MODERN PHYSICS UNIT- MODERN PHYSICS Introduction to blackbody radiation spectrum: A body wic absorbs all radiation tat is incident on it is called a perfect blackbody. Wen radiation allowed to fall on suc a body, it

More information

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

Exam 2 Thursday (7:30-9pm) It will cover material through HW 7, but no material that was on the 1 st exam. Exam 2 Thursday (7:30-9pm) It will covr matrial through HW 7, but no matrial that was on th 1 st xam. What happns if w bash atoms with lctrons? In atomic discharg lamps, lots of lctrons ar givn kintic

More information

Gamma-ray burst spectral evolution in the internal shock model

Gamma-ray burst spectral evolution in the internal shock model Gamma-ray burst spctral volution in th intrnal shock modl in collaboration with: Žljka Marija Bošnjak Univrsity of Rijka, Croatia Frédéric Daign (Institut d Astrophysiqu d Paris) IAU$Symposium$324$0$Ljubljana,$Sptmbr$2016$

More information

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)

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) NUCLEAR AND PARTICLE PHYSICS NET/JRF (JUNE-) 64 Q. Th radius of a 9Cu nuclus is masurd to b 4.8 - cm. (A). Th radius of a 7 Mg nuclus can b stimatd to b.86 - cm (b) 5. - cm (c).6 - cm (d) 8.6 - cm (c)

More information

2. Laser physics - basics

2. Laser physics - basics . Lasr physics - basics Spontanous and stimulatd procsss Einstin A and B cofficints Rat quation analysis Gain saturation What is a lasr? LASER: Light Amplification by Stimulatd Emission of Radiation "light"

More information

λ = 2L n Electronic structure of metals = 3 = 2a Free electron model Many metals have an unpaired s-electron that is largely free

λ = 2L n Electronic structure of metals = 3 = 2a Free electron model Many metals have an unpaired s-electron that is largely free 5.6 4 Lctur #4-6 pag Elctronic structur of mtals r lctron modl Many mtals av an unpaird s-lctron tat is largly fr Simplst modl: Particl in a box! or a cubic box of lngt L, ψ ( xyz) 8 xπ ny L L L n x π

More information

Single electron experiments in quantum conductors : the on-demand single electron source the charge relaxation resistance

Single electron experiments in quantum conductors : the on-demand single electron source the charge relaxation resistance Singl lctron xprimnts in quantum conductors : th on-dmand singl lctron sourc th charg rlaxation rsistanc «DEG tam» Laboratoir Pirr Aigrain, Ecol Normal Supériur Sampls : Y. Jin, A. avanna, B. Etinn (LPN-NRS

More information

Classical Magnetic Dipole

Classical Magnetic Dipole Lctur 18 1 Classical Magntic Dipol In gnral, a particl of mass m and charg q (not ncssarily a point charg), w hav q g L m whr g is calld th gyromagntic ratio, which accounts for th ffcts of non-point charg

More information

Chapter 30: Quantum Physics

Chapter 30: Quantum Physics Answrs to Evn-Numbrd Concptual Qustions. I nrgy is quantizd, as suggstd by Planck, t amount o nrgy or vn a singl ig-rquncy poton can b arbitrarily larg. T init nrgy in a blackbody simply can t produc suc

More information

fiziks Institute for NET/JRF, GATE, IIT JAM, M.Sc. Entrance, JEST, TIFR and GRE in Physics

fiziks Institute for NET/JRF, GATE, IIT JAM, M.Sc. Entrance, JEST, TIFR and GRE in Physics Atoic and olcular Physics JEST Q. Th binding nrgy of th hydrogn ato (lctron bound to proton) is.6 V. Th binding nrgy of positroniu (lctron bound to positron) is (a).6 / V (b).6 / 8 V (c).6 8 V (d).6 V.6

More information

Precise Masses of particles

Precise Masses of particles /1/15 Physics 1 April 1, 15 Ovrviw of topic Th constitunts and structur of nucli Radioactivity Half-lif and Radioactiv dating Nuclar Binding Enrgy Nuclar Fission Nuclar Fusion Practical Applications of

More information

A Propagating Wave Packet Group Velocity Dispersion

A Propagating Wave Packet Group Velocity Dispersion Lctur 8 Phys 375 A Propagating Wav Packt Group Vlocity Disprsion Ovrviw and Motivation: In th last lctur w lookd at a localizd solution t) to th 1D fr-particl Schrödingr quation (SE) that corrsponds to

More information

Chapter 10: Wave Properties of Particles

Chapter 10: Wave Properties of Particles Chapter 10: Wave Properties of Particles Particles such as electrons may demonstrate wave properties under certain conditions. The electron microscope uses these properties to produce magnified images

More information

Radiation Physics Laboratory - Complementary Exercise Set MeBiom 2016/2017

Radiation Physics Laboratory - Complementary Exercise Set MeBiom 2016/2017 Th following qustions ar to b answrd individually. Usful information such as tabls with dtctor charactristics and graphs with th proprtis of matrials ar availabl in th cours wb sit: http://www.lip.pt/~patricia/fisicadaradiacao.

More information

Disorder and mesoscopic physics. Lecture 2. Quantum transport, Landauer-Büttiker weak-localization G 2. Landauer-Büttiker formulae.

Disorder and mesoscopic physics. Lecture 2. Quantum transport, Landauer-Büttiker weak-localization G 2. Landauer-Büttiker formulae. isordr and msoscopic pysics Landaur-Büttikr formula Lctur wo-trminal conductanc G Quantum transport, Landaur-Büttikr wak-localization our-trminal conductanc non-invasiv voltag probs R Gills Montambaux,

More information

Spatial channeling of energy and momentum of energetic ions by destabilized Alfvén eigenmodes

Spatial channeling of energy and momentum of energetic ions by destabilized Alfvén eigenmodes Spatial channling of nrgy and momntum of nrgtic ions by dstabilizd Alfvén ignmods Ya.I. Kolsnichnko 1,V.V. Lutsnko 1, R.B. Whit, Yu.V. Yakovnko 1 1 Institut for Nuclar Rsarch, Kyiv, Ukrain Princton Plasma

More information

Lecture 18 - Semiconductors - continued

Lecture 18 - Semiconductors - continued Lctur 18 - Smiconductors - continud Lctur 18: Smiconductors - continud (Kittl C. 8) + a - Donors and accptors Outlin Mor on concntrations of lctrons and ols in Smiconductors Control of conductivity by

More information

BETA DECAY VISUAL PHYSICS ONLINE

BETA DECAY VISUAL PHYSICS ONLINE VISUAL PHYSICS ONLINE BETA DECAY Suppos now that a nuclus xists which has ithr too many or too fw nutrons rlativ to th numbr of protons prsnt for stability. Stability can b achivd by th convrsion insid

More information

Phys 446: Solid State Physics / Optical Properties. Lattice vibrations: Thermal, acoustic, and optical properties. Fall v =

Phys 446: Solid State Physics / Optical Properties. Lattice vibrations: Thermal, acoustic, and optical properties. Fall v = Phys 446: Solid Stat Physics / Optical Proprtis Lattic vibrations: Thrmal, acoustic, and optical proprtis Solid Stat Physics Last wk: (Ch. 3) Phonons Today: Einstin and Dby modls for thrmal capacity Thrmal

More information

Chemical Engineering 412

Chemical Engineering 412 Chical Enginring 4 Introductory Nuclar Enginring Lctur 6 Nuclar Radiation Typs Ky oints Typs of cay Na roprtis athatical scriptions Cavats cay Charts (KNOW HOW TO USE!) Nuclar Equation for cay -Valus for

More information

On the Hamiltonian of a Multi-Electron Atom

On the Hamiltonian of a Multi-Electron Atom On th Hamiltonian of a Multi-Elctron Atom Austn Gronr Drxl Univrsity Philadlphia, PA Octobr 29, 2010 1 Introduction In this papr, w will xhibit th procss of achiving th Hamiltonian for an lctron gas. Making

More information

Particles and Waves Particles Waves

Particles and Waves Particles Waves Particles and Waves Particles Discrete and occupy space Exist in only one location at a time Position and velocity can be determined with infinite accuracy Interact by collisions, scattering. Waves Extended,

More information

Derivation of Electron-Electron Interaction Terms in the Multi-Electron Hamiltonian

Derivation of Electron-Electron Interaction Terms in the Multi-Electron Hamiltonian Drivation of Elctron-Elctron Intraction Trms in th Multi-Elctron Hamiltonian Erica Smith Octobr 1, 010 1 Introduction Th Hamiltonian for a multi-lctron atom with n lctrons is drivd by Itoh (1965) by accounting

More information

Structure of the Atom. Thomson s Atomic Model. Knowledge of atoms in Experiments of Geiger and Marsden 2. Experiments of Geiger and Marsden

Structure of the Atom. Thomson s Atomic Model. Knowledge of atoms in Experiments of Geiger and Marsden 2. Experiments of Geiger and Marsden CHAPTER 4 Structur of th Atom 4.1 Th Atomic Modls of Thomson and Ruthrford 4. Ruthrford Scattring 4.3 Th Classic Atomic Modl 4.4 Th Bohr Modl of th Hydrogn Atom 4.5 Succsss & Failurs of th Bohr Modl 4.6

More information

Problem Set 4 Solutions Distributed: February 26, 2016 Due: March 4, 2016

Problem Set 4 Solutions Distributed: February 26, 2016 Due: March 4, 2016 Probl St 4 Solutions Distributd: Fbruary 6, 06 Du: March 4, 06 McQuarri Probls 5-9 Ovrlay th two plots using Excl or Mathatica. S additional conts blow. Th final rsult of Exapl 5-3 dfins th forc constant

More information

Addition of angular momentum

Addition of angular momentum Addition of angular momntum April, 0 Oftn w nd to combin diffrnt sourcs of angular momntum to charactriz th total angular momntum of a systm, or to divid th total angular momntum into parts to valuat th

More information

High Energy Astrophysics

High Energy Astrophysics High Enrg Astrophsics Radiation Procsss /4 Giampaolo Pisano Jodrll Bank Cntr for Astrophsics - Univrsit of Manchstr giampaolo.pisano@manchstr.ac.uk Fbruar 1 Radiation Procsss Rfrncs: - Brmsstrahlung -

More information

Neutrino Physics. Caren Hagner, Universität Hamburg

Neutrino Physics. Caren Hagner, Universität Hamburg Nutrino Physics Carn Hagnr, Univrsität Hamburg What ar nutrinos? Nutrino mass and mixing Nutrino oscillations Nutrino bams: OPERA Oscillation of acclrator nutrinos Solar Nutrinos: BOREXINO (KamLAND ractor

More information

Lecture contents. Bloch theorem k-vector Brillouin zone Almost free-electron model Bands Effective mass Holes. NNSE 508 EM Lecture #9

Lecture contents. Bloch theorem k-vector Brillouin zone Almost free-electron model Bands Effective mass Holes. NNSE 508 EM Lecture #9 Lctur contnts Bloch thorm -vctor Brillouin zon Almost fr-lctron modl Bnds ffctiv mss Hols Trnsltionl symmtry: Bloch thorm On-lctron Schrödingr qution ch stt cn ccommo up to lctrons: If Vr is priodic function:

More information

The Photoelectric Effect

The Photoelectric Effect Stellar Astrophysics: The Interaction of Light and Matter The Photoelectric Effect Methods of electron emission Thermionic emission: Application of heat allows electrons to gain enough energy to escape

More information

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

Chemical Physics II. More Stat. Thermo Kinetics Protein Folding... Chmical Physics II Mor Stat. Thrmo Kintics Protin Folding... http://www.nmc.ctc.com/imags/projct/proj15thumb.jpg http://nuclarwaponarchiv.org/usa/tsts/ukgrabl2.jpg http://www.photolib.noaa.gov/corps/imags/big/corp1417.jpg

More information

The Relativistic Stern-Gerlach Force C. Tschalär 1. Introduction

The Relativistic Stern-Gerlach Force C. Tschalär 1. Introduction Th Rlativistic Strn-Grlach Forc C. Tschalär. Introduction For ovr a dcad, various formulations of th Strn-Grlach (SG) forc acting on a particl with spin moving at a rlativistic vlocity in an lctromagntic

More information

DIS-Parity. Search for New Physics Through Parity Violation In Deep Inelastic Electron Scattering. The Physics Case

DIS-Parity. Search for New Physics Through Parity Violation In Deep Inelastic Electron Scattering. The Physics Case DIS-Parity Sarch for Nw Physics Through Parity Violation In Dp Inlastic Elctron Scattring Th Physics Cas R. Arnold for th DIS-Parity Collaboration Exprimnt Plan by Stv Rock will follow 12 Jun 2003 DIS-Parity

More information

Quantitative Model of Unilluminated Diode part II. G.R. Tynan UC San Diego MAE 119 Lecture Notes

Quantitative Model of Unilluminated Diode part II. G.R. Tynan UC San Diego MAE 119 Lecture Notes Quantitativ Modl of Unilluminatd Diod part II G.R. Tynan UC San Digo MAE 119 Lctur Nots Minority Carrir Dnsity at dg of quasinutral rgion incrass EXPONENTIALLY forward bias p nb n pa = p n0 xp qv a kt

More information

Introduction. Learning Objectives. On completion of this chapter you will be able to:

Introduction. Learning Objectives. On completion of this chapter you will be able to: Introduction Learning Objectives On completion of tis capter you will be able to: 1. Define Compton Effect. 2. Derive te sift in incident ligt wavelengt and Compton wavelengt. 3. Explain ow te Compton

More information

Simulations des micro-décharges de type MHCD

Simulations des micro-décharges de type MHCD Simulations ds micro-déchargs d typ MHCD Lann Pitchford Group GREPHE Laboratoir ds Plasmas t Convrsion d Enrgi Univrsité d Toulous t CNRS UMR 5213 pitchford@laplac.univ-tls.fr JP Bouf, G. Haglaar, Th Callgari

More information

Addition of angular momentum

Addition of angular momentum Addition of angular momntum April, 07 Oftn w nd to combin diffrnt sourcs of angular momntum to charactriz th total angular momntum of a systm, or to divid th total angular momntum into parts to valuat

More information

Sinusoidal Response Notes

Sinusoidal Response Notes ECE 30 Sinusoidal Rspons Nots For BIBO Systms AStolp /29/3 Th sinusoidal rspons of a systm is th output whn th input is a sinusoidal (which starts at tim 0) Systm Sinusoidal Rspons stp input H( s) output

More information

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

Standard Model - Electroweak Interactions. Standard Model. Outline. Weak Neutral Interactions. Electroweak Theory. Experimental Tests. Standard Modl - Elctrowak Intractions Outlin ak Nutral Intractions Nutral Currnts (NC) Elctrowak Thory ± and Z and γ Discovry of ± Exprimntal Tsts LEP Z Boson Mass and idth Numbr of Nutrinos ± Boson ±

More information

Collisions between electrons and ions

Collisions between electrons and ions DRAFT 1 Collisions btwn lctrons and ions Flix I. Parra Rudolf Pirls Cntr for Thortical Physics, Unirsity of Oxford, Oxford OX1 NP, UK This rsion is of 8 May 217 1. Introduction Th Fokkr-Planck collision

More information

PHYS 3313 Section 001 Lecture #16

PHYS 3313 Section 001 Lecture #16 PHYS 3313 Section 001 Lecture #16 Monday, Mar. 24, 2014 De Broglie Waves Bohr s Quantization Conditions Electron Scattering Wave Packets and Packet Envelops Superposition of Waves Electron Double Slit

More information

Coupled Pendulums. Two normal modes.

Coupled Pendulums. Two normal modes. Tim Dpndnt Two Stat Problm Coupld Pndulums Wak spring Two normal mods. No friction. No air rsistanc. Prfct Spring Start Swinging Som tim latr - swings with full amplitud. stationary M +n L M +m Elctron

More information

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

26-Sep-16. Nuclear energy production. Nuclear energy production. Nuclear energy production. Nuclear energy production Aim: valuat nrgy-gnration rat pr unit mass. Sun: (chck L /M, human ) nrgy-gnration rat producd from fusion of two nucli a + A: nrgy rlasd pr raction raction rat pr unit volum (includs cross sction and

More information

PRINCIPLES OF PLASMA PROCESSING Course Notes: Prof. J. P. Chang Part B3: ATOMIC COLLISIONS AND SPECTRA

PRINCIPLES OF PLASMA PROCESSING Course Notes: Prof. J. P. Chang Part B3: ATOMIC COLLISIONS AND SPECTRA Atomic Collisions and Spctra 125 PRINCIPLES OF PLASMA PROCESSING Cours Nots: Prof. J. P. Chang Part B3: ATOMIC COLLISIONS AND SPECTRA I. ATOMIC ENERGY LEVELS Atoms and molculs mit lctromagntic radiation

More information

ELECTRON-MUON SCATTERING

ELECTRON-MUON SCATTERING ELECTRON-MUON SCATTERING ABSTRACT Th lctron charg is considrd to b distributd or xtndd in spac. Th diffrntial of th lctron charg is st qual to a function of lctron charg coordinats multiplid by a four-dimnsional

More information

Prelab Lecture Chmy 374 Thur., March 22, 2018 Edited 22mar18, 21mar18

Prelab Lecture Chmy 374 Thur., March 22, 2018 Edited 22mar18, 21mar18 Prlab Lctur Cmy 374 Tur., Marc, 08 Editd mar8, mar8 LA REPORT:From t ClassicalTrmoISub-7.pdf andout: Was not a dry lab A partially complt spradst was postd on wb Not ruird 3 If solid is pur X Partial

More information

Quantitative Model of PV Cells The Illuminated Diode. G.R. Tynan UC San Diego MAE 119 Lecture Notes

Quantitative Model of PV Cells The Illuminated Diode. G.R. Tynan UC San Diego MAE 119 Lecture Notes Quantitativ Modl of PV Clls T Illuminatd Diod G.R. Tynan UC San Digo MAE 119 ctur Nots WE FOUND WHAT WE SEEK: JJ(V) Currnt Dnsity vs Voltag Across Diod: J total qdn p qd pn J + J kt ( xp( qv / ) 1) 0 0

More information