Lecture #2: Wave Nature of the Electron and the Internal Structure of an Atom

Size: px
Start display at page:

Download "Lecture #2: Wave Nature of the Electron and the Internal Structure of an Atom"

Transcription

1 5.61 Fall 013 Lctur # pag 1 Lctur #: Wav Natur of t Elctro ad t Itral Structur of a Atom Last tim: Surpris Ligt as particl 1. Potolctric ffct, spcially KE vs. ν. Ligt as packts of rgy, calld potos, E = ν.. Compto scattrig Ligt as avig bot KE (scalar) ad p (vctor). Billiard-lik scattrig of poto by Today: 1. Aotr surpris wav caractr of compar diffractio of X-ray ad by sam Al foil masur λ = p dbrogli postulatd, for objcts cosidrd to b particls (.g. ) tat λ = p. Itral structur of mattr: mostly mpty spac! I ordr to fill spac Rutrford postulatd platary atom * radiativ collaps (a fatal flaw) Bor modl * postulatd quatizd (ad cosrvd) agular momtum f = * Explaid li spctrum of H * radiativ collaps avoidd d Brogli * itgr # of λ aroud Bor orbit to prvt aiilatio of t by dstructiv itrfrc X-ray ad diffractio off of Al foil rvisd 9/9/13 9:9:00 AM

2 5.61 Fall 013 Lctur # pag OR X-ray Bam bam Bam stop targt fluorsct Al foil scr Us kow lattic spacigs i Al as a rulr to masur λ of S Figur 1.13 i McQuarri, pag 30. Obtai bull s y diffractio pattr for bot X-ray ad. Pairs of rigs com from scattrig off arst ad scod arst igbor atoms. Ca coos λ of X-rays (masurd i sparat xprimt). p, p = m q V 1/. Ca cotrol p of : E = q V = m W t rig pattrs matc, must av t sam λ as X-rays (λ is a way to masur λ, w fid tat it is λ =. p small p, larg λ larg p, small λ x-ray =λ ). Tis How dos diffractio work? No-Lctur 1/ a a a is uit cll distac a rvisd 9/9/13 9:9:00 AM

3 5.61 Fall 013 Lctur # pag 3 S pag 59 of Karplus ad Portr. λ icidt bam (pla wav) θ θ θ diffractd bam a Gt costructiv itrfrc from scattrig off of atoms sparatd by a w t agl θ btw icidt ad dtctd radiatio is suc tat t pats diffr by λ. ( is a itgr, t ordr ) Suppos λ = a/ arst igbor a si θ arst igbor a θ d arst igbor 1/ a si θ 1/ a λ = asiθ 1 st ordr w = 1 λ = 1/ asiθ λ θ = si 1 1 st ordr w = 1 a d arst igbor θ = si 1 θ = si 1 3/ = 1 θ 1 = 0.5 θ 1 = 0.36 = θ = 1.57 θ = 0.79 θ = si 1 θ λ 1/ a T 1 st -ordr rig for t scod arst igbor is of smallr diamtr ta tat for t arst igbor. rvisd 9/9/13 9:9:00 AM

4 5.61 Fall 013 Lctur # pag 4 T agular sparatio btw rig pairs is largr i scod ordr. [Tis rmids you tat a gratig opratd i scod ordr givs igr spctral rsolutio ta i first ordr.] Diffrt rig pattrs (spacigs ad rlativ itsitis) ar obsrvd for simpl cubic fac-ctrd cubic body-ctrd cubic xagoal clos packd SC FCC BCC HCP Ca us powdr pattr to assig uit cll typ ad to dtrmi t uit cll distacs. Wy is it calld it a powdr pattr? END of NON-LECTURE So w ca masur a usig X-rays of kow λ. W ca t masur λ of for masurd p (masurd i a sparat xprimt). Fid mpirically tat λ = p. Eisti (1906 spcial rlativity) sowd, for ligt E ν p = = =. c λν λ DBrogli, i is 194 P.D. Tsis, postulatd tat if p = for ligt, t t sam λ formula would giv λ for particls. Was tis just a good guss or a dp isigt? Exampl calculatio ad a paradox For a, if λ = 1Å, t v =? E =? Typical diamtr of a atom is ~1Å. Wat E or v of a orbitig lctro would b rquird for a to liv isid a atom? J s λ = m = = Tus, for λ = 1Å, w prdict p ( ). 31 kg)(v[m / s] v = m / s.4% of c (spd of ligt). E = 1 mv = J = ( V / J )( J ) (uits covrsio) = 149V 10 typical ioizatio rgy! (Ergy rquird to rmov o from a gas pas atom or molcul.) rvisd 9/9/13 9:9:00 AM

5 5.61 Fall 013 Lctur # pag 5 Paradox: How ca fit isid of a atom? Typical diamtr of a atom is ~1Å. Typical bidig rgy of to uclus is 15V. Yt w rquir tat, for a to av small oug λ to fit isid a atom, it must av a rgy 10 too larg to rmai trappd isid t atom. Tis is a paradox. To udrstad tis w must go back to t qustio: wat is t itral structur of a atom? Erst Rutrford 1911 α-particl scattrig off a mtal foil. Exprimts by Has Gigr ad Erst Marsd. α-particl (H + + io io) back-scattr dtctor scr ti foil forward-scattr dtctor dtctor scr scr Foud tat vry fw α-particls wr back-scattrd. If atoms wr omogous ad w kow t # of atoms pr ara of foil (ow would w kow tis?), w kow tat most of t α particls sould arriv at t dtctor scr udflctd or oly wakly. Fractio backscattrd tlls us t ffctiv diamtr, mass, ad carg of ac atom, as s by a α particl. Foud t atomic diamtr dtrmid i tis way to b vastly smallr ta t distac btw atoms (calculatd from t masurd dsity of t mtal of t foil ad its kow atomic wigt). Jllium (omogous atom) is ruld out. Most of mass of atom is localizd isid a vry small diamtr uclus. Yt atoms ar spac fillig. [Also, t carg o tis uclus is positiv ad qual to t atomic umbr of t atom.] rvisd 9/9/13 9:9:00 AM

6 5.61 Fall 013 Lctur # pag 6 How do w ratioaliz ts two smigly cotradictory facts? Platary modl of a atom proposd by Rutrford: orbit + uclus Coulomb attractio btw uclus ad : Ctrifugal forc: F i = F out, solv for v F q 1 r = i SI uits, ε 0 is prmittivity (1) 4πε 0 of fr spac m v F out =+ () r q 1 1/ v = 4πε 0 m r. (3) W av (tratig uclus as ifiitly avy), for vry valu of t circular orbit radius, r, a costat spd, v, alog t orbit. No quatizatio of r, v, or E is rquird, but small r must corrspod to larg v. W av a acclratd carg radiats rgy = ν wr ν is t frqucy of t orbital motio. Loss rgy. Must mov to smallr radius orbit. Orbit frqucy icrass. Rat of radiatio of rgy icrass. Radiativ collaps. Bad! Ca tis cotradictio b xplaid? rvisd 9/9/13 9:9:00 AM

7 5.61 Fall 013 Lctur # pag 7 circumfrc = π r π r priod = v v q 1 frqucy= = 3 πr rπε 0 m 4π r small r, ig frqucy spirals i toward uclus. No-Lctur ν t To avoid tis fatal flaw, Bor postulatd tat lctro agular momtum, f, is quatizd, ad trfor, cosrvd. f = r p = m vr = (4) v = r p m r Tis provids a artificial aswr to t problm of radiativ collaps. Wy artificial? Combi Eqs. (3) ad (4) to solv for t orbit radius: Orbit radius, r, gts larg as 4πε r 0 = = [0.59 q 059 ]Å m f atomic uit of lgt (or ) icrass. Istad, solv for t orbit vlocity: 1 q 1 v = = [ ]m / s 4πε 0 v gts small as f (or ) icrass. Nxt, solv for λ : 1 q m p = 4πε 0 8π ε 0 π r λ = = = = [3.3]Å p q m Circumfrc of t orbit = πr = λ! Tis is a plasat surpris. T fits isid a atom if its wavlgt is arragd alog t orbit circumfrc! Nxt, solv for t allowd rgy lvls: rvisd 9/9/13 9:9:00 AM

8 5.61 Fall 013 Lctur # pag 8 1 q 1 E = T r ( )+ V(r ) = m v 4πε 0 r 4 m q 1 = 8ε 0 I I Rydbrg costat for H cr H Balmr, from umrical study of t missio lis of H atom, proposd tat t frqucy 1 of a spctral li is giv by tims t diffrc btw rgy lvls. Trasitios btw discrt (quatizd) rgy lvls! ' Turs out tat ν ', = E ' E * Tis rgy lvl formula for t Bor atom xactly rproducs all of t rgy m m uclus lvls of all 1 systms rplacig m by μ = m m + m uclus * accouts for li spctra if ν =, E E * accordig to Bor t lowst possibl valu of f is f = 1 (w will fid out latr tat f = 0 is also possibl) * dos ot accout for rlativ itsitis of spctral lis, or radiativ liftims of rgy lvls * dos ot xplai ffct of a magtic fild o spctrum * mor satisfyig to us dbrogli s ida to prvt radiativ collaps. But isistc o itgr orbital agular momta [Bor] ad avoidac of dstructiv itrfrc aroud a circular orbit [d Brogli] ar bot artificial idas. * if t is movig o a circular orbit, it must radiat, but is it rally movig? WEIRD! dbrogli: Itgr umbr of λ aroud orbit circumfrc is wat is rquird to prvt dstructiv itrfrc of wit itslf. A sould ot disappar. Sms mor fudamtal. But w ar just makig ad oc proposals to xplai a fudamtal cotradictio. W sould ot b comfortabl wit ay of tis! Bor tory caot xplai ay spctra otr ta 1 spctra. At tis stag, t spctrum of t simplst possibl atom, H, rmais a mystry. rvisd 9/9/13 9:9:00 AM

9 5.61 Fall 013 Lctur # pag 9 Wat do w do ow? Nxt Lctur: Discuss wav quatio i prparatio for Scrödigr Equatio, wic is a mor complt ad widly applicabl way to dal wit ts uxpctd rsults. rvisd 9/9/13 9:9:00 AM

10 MIT OpCoursWar ttp://ocw.mit.du 5.61 Pysical Cmistry Fall 013 For iformatio about citig ts matrials or our Trms of Us, visit: ttp://ocw.mit.du/trms.

8(4 m0) ( θ ) ( ) Solutions for HW 8. Chapter 25. Conceptual Questions

8(4 m0) ( θ ) ( ) Solutions for HW 8. Chapter 25. Conceptual Questions Solutios for HW 8 Captr 5 Cocptual Qustios 5.. θ dcrass. As t crystal is coprssd, t spacig d btw t plas of atos dcrass. For t first ordr diffractio =. T Bragg coditio is = d so as d dcrass, ust icras for

More information

Physics 2D Lecture Slides Lecture 14: Feb 3 rd 2004

Physics 2D Lecture Slides Lecture 14: Feb 3 rd 2004 Bria Wcht, th TA is back! Pl. giv all rgrad rqusts to him Quiz 4 is This Friday Physics D Lctur Slids Lctur 14: Fb 3 rd 004 Vivk Sharma UCSD Physics Whr ar th lctros isid th atom? Early Thought: Plum puddig

More information

Session : Plasmas in Equilibrium

Session : Plasmas in Equilibrium Sssio : Plasmas i Equilibrium Ioizatio ad Coductio i a High-prssur Plasma A ormal gas at T < 3000 K is a good lctrical isulator, bcaus thr ar almost o fr lctros i it. For prssurs > 0.1 atm, collisio amog

More information

Blackbody Radiation. All bodies at a temperature T emit and absorb thermal electromagnetic radiation. How is blackbody radiation absorbed and emitted?

Blackbody Radiation. All bodies at a temperature T emit and absorb thermal electromagnetic radiation. How is blackbody radiation absorbed and emitted? All bodis at a tmpratur T mit ad absorb thrmal lctromagtic radiatio Blackbody radiatio I thrmal quilibrium, th powr mittd quals th powr absorbd How is blackbody radiatio absorbd ad mittd? 1 2 A blackbody

More information

coulombs or esu charge. It s mass is about 1/1837 times the mass of hydrogen atom. Thus mass of electron is

coulombs or esu charge. It s mass is about 1/1837 times the mass of hydrogen atom. Thus mass of electron is 1 ATOMIC STRUCTURE Fudamtal Particls: Mai Fudamtal Particl : (a) Elctro: It is a fudamtal particl of a atom which carris a uit gativ charg. It was discovrd by J.J. Thomso (1897) from th studis carrid out

More information

Chapter Taylor Theorem Revisited

Chapter Taylor Theorem Revisited Captr 0.07 Taylor Torm Rvisitd Atr radig tis captr, you sould b abl to. udrstad t basics o Taylor s torm,. writ trascdtal ad trigoomtric uctios as Taylor s polyomial,. us Taylor s torm to id t valus o

More information

They must have different numbers of electrons orbiting their nuclei. They must have the same number of neutrons in their nuclei.

They must have different numbers of electrons orbiting their nuclei. They must have the same number of neutrons in their nuclei. 37 1 How may utros ar i a uclus of th uclid l? 20 37 54 2 crtai lmt has svral isotops. Which statmt about ths isotops is corrct? Thy must hav diffrt umbrs of lctros orbitig thir ucli. Thy must hav th sam

More information

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

Blackbody Radiation. All bodies at a temperature T emit and absorb thermal electromagnetic radiation. How is blackbody radiation absorbed and emitted?

Blackbody Radiation. All bodies at a temperature T emit and absorb thermal electromagnetic radiation. How is blackbody radiation absorbed and emitted? All bodis at a tmpratur T mit ad absorb thrmal lctromagtic radiatio Blackbody radiatio I thrmal quilibrium, th powr mittd quals th powr absorbd How is blackbody radiatio absorbd ad mittd? 1 2 A blackbody

More information

5.1 The Nuclear Atom

5.1 The Nuclear Atom Sav My Exams! Th Hom of Rvisio For mor awsom GSE ad lvl rsourcs, visit us at www.savmyxams.co.uk/ 5.1 Th Nuclar tom Qustio Papr Lvl IGSE Subjct Physics (0625) Exam oard Topic Sub Topic ooklt ambridg Itratioal

More information

Partition Functions and Ideal Gases

Partition Functions and Ideal Gases Partitio Fuctios ad Idal Gass PFIG- You v lard about partitio fuctios ad som uss ow w ll xplor tm i mor dpt usig idal moatomic diatomic ad polyatomic gass! for w start rmmbr: Q( N ( N! N Wat ar N ad? W

More information

Probability & Statistics,

Probability & Statistics, Probability & Statistics, BITS Pilai K K Birla Goa Campus Dr. Jajati Kshari Sahoo Dpartmt of Mathmatics BITS Pilai, K K Birla Goa Campus Poisso Distributio Poisso Distributio: A radom variabl X is said

More information

Bohr type models of the atom give a totally incorrect picture of the atom and are of only historical significance.

Bohr type models of the atom give a totally incorrect picture of the atom and are of only historical significance. VISUAL PHYSICS ONLIN BOHR MODL OF TH ATOM Bhr typ mdls f th atm giv a ttally icrrct pictur f th atm ad ar f ly histrical sigificac. Fig.. Bhr s platary mdl f th atm. Hwvr, th Bhr mdls wr a imprtat stp

More information

LECTURE 13 Filling the bands. Occupancy of Available Energy Levels

LECTURE 13 Filling the bands. Occupancy of Available Energy Levels LUR 3 illig th bads Occupacy o Availabl rgy Lvls W hav dtrmid ad a dsity o stats. W also d a way o dtrmiig i a stat is illd or ot at a giv tmpratur. h distributio o th rgis o a larg umbr o particls ad

More information

(Reference: sections in Silberberg 5 th ed.)

(Reference: sections in Silberberg 5 th ed.) ALE. Atomic Structur Nam HEM K. Marr Tam No. Sctio What is a atom? What is th structur of a atom? Th Modl th structur of a atom (Rfrc: sctios.4 -. i Silbrbrg 5 th d.) Th subatomic articls that chmists

More information

From Classical to Quantum mechanics

From Classical to Quantum mechanics From Classical to Quantum mcanics Engl & Rid 99-300 vrij Univrsitit amstrdam Classical wav baviour Ligt is a wav Two-slit xprimnt wit potons (81-85) 1 On sourc Intrfrnc sourcs ttp://www.falstad.com/matpysics.tml

More information

z 1+ 3 z = Π n =1 z f() z = n e - z = ( 1-z) e z e n z z 1- n = ( 1-z/2) 1+ 2n z e 2n e n -1 ( 1-z )/2 e 2n-1 1-2n -1 1 () z

z 1+ 3 z = Π n =1 z f() z = n e - z = ( 1-z) e z e n z z 1- n = ( 1-z/2) 1+ 2n z e 2n e n -1 ( 1-z )/2 e 2n-1 1-2n -1 1 () z Sris Expasio of Rciprocal of Gamma Fuctio. Fuctios with Itgrs as Roots Fuctio f with gativ itgrs as roots ca b dscribd as follows. f() Howvr, this ifiit product divrgs. That is, such a fuctio caot xist

More information

Atomic Physics 4. Name: Date: 1. The de Broglie wavelength associated with a car moving with a speed of 20 m s 1 is of the order of. A m.

Atomic Physics 4. Name: Date: 1. The de Broglie wavelength associated with a car moving with a speed of 20 m s 1 is of the order of. A m. Name: Date: Atomic Pysics 4 1. Te de Broglie wavelegt associated wit a car movig wit a speed of 0 m s 1 is of te order of A. 10 38 m. B. 10 4 m. C. 10 4 m. D. 10 38 m.. Te diagram below sows tree eergy

More information

MONTGOMERY COLLEGE Department of Mathematics Rockville Campus. 6x dx a. b. cos 2x dx ( ) 7. arctan x dx e. cos 2x dx. 2 cos3x dx

MONTGOMERY COLLEGE Department of Mathematics Rockville Campus. 6x dx a. b. cos 2x dx ( ) 7. arctan x dx e. cos 2x dx. 2 cos3x dx MONTGOMERY COLLEGE Dpartmt of Mathmatics Rockvill Campus MATH 8 - REVIEW PROBLEMS. Stat whthr ach of th followig ca b itgratd by partial fractios (PF), itgratio by parts (PI), u-substitutio (U), or o of

More information

Outline. Ionizing Radiation. Introduction. Ionizing radiation

Outline. Ionizing Radiation. Introduction. Ionizing radiation Outli Ioizig Radiatio Chaptr F.A. Attix, Itroductio to Radiological Physics ad Radiatio Dosimtry Radiological physics ad radiatio dosimtry Typs ad sourcs of ioizig radiatio Dscriptio of ioizig radiatio

More information

Problem Value Score Earned No/Wrong Rec -3 Total

Problem Value Score Earned No/Wrong Rec -3 Total GEORGIA INSTITUTE OF TECHNOLOGY SCHOOL of ELECTRICAL & COMPUTER ENGINEERING ECE6 Fall Quiz # Writt Eam Novmr, NAME: Solutio Kys GT Usram: LAST FIRST.g., gtiit Rcitatio Sctio: Circl t dat & tim w your Rcitatio

More information

1985 AP Calculus BC: Section I

1985 AP Calculus BC: Section I 985 AP Calculus BC: Sctio I 9 Miuts No Calculator Nots: () I this amiatio, l dots th atural logarithm of (that is, logarithm to th bas ). () Ulss othrwis spcifid, th domai of a fuctio f is assumd to b

More information

PURE MATHEMATICS A-LEVEL PAPER 1

PURE MATHEMATICS A-LEVEL PAPER 1 -AL P MATH PAPER HONG KONG EXAMINATIONS AUTHORITY HONG KONG ADVANCED LEVEL EXAMINATION PURE MATHEMATICS A-LEVEL PAPER 8 am am ( hours) This papr must b aswrd i Eglish This papr cosists of Sctio A ad Sctio

More information

Physics of the Interstellar and Intergalactic Medium

Physics of the Interstellar and Intergalactic Medium PYA0 Sior Sophistr Physics of th Itrstllar ad Itrgalactic Mdium Lctur 7: II gios Dr Graham M. arpr School of Physics, TCD Follow-up radig for this ad t lctur Chaptr 5: Dyso ad Williams (lss dtaild) Chaptr

More information

to the SCHRODINGER EQUATION The case of an electron propagating in a crystal lattice

to the SCHRODINGER EQUATION The case of an electron propagating in a crystal lattice Lctur Nots PH 411/511 ECE 598 A. La Rosa INTRODUCTION TO QUANTUM MECHANICS CHAPTER-9 From th HAMILTONIAN EQUATIONS to th SCHRODINGER EQUATION Th cas of a lctro propagatig i a crystal lattic 9.1 Hamiltoia

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

APPENDIX: STATISTICAL TOOLS

APPENDIX: STATISTICAL TOOLS I. Nots o radom samplig Why do you d to sampl radomly? APPENDI: STATISTICAL TOOLS I ordr to masur som valu o a populatio of orgaisms, you usually caot masur all orgaisms, so you sampl a subst of th populatio.

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

Physics 302 Exam Find the curve that passes through endpoints (0,0) and (1,1) and minimizes 1

Physics 302 Exam Find the curve that passes through endpoints (0,0) and (1,1) and minimizes 1 Physis Exam 6. Fid th urv that passs through dpoits (, ad (, ad miimizs J [ y' y ]dx Solutio: Si th itgrad f dos ot dpd upo th variabl of itgratio x, w will us th sod form of Eulr s quatio: f f y' y' y

More information

Terahertz band-gap in InAs/GaSb type II superlattices

Terahertz band-gap in InAs/GaSb type II superlattices Trart Scic ad Tcology, ISSN 1941-7411 Vol.1, No 4, Dcmbr 008 Trart bad-gap i IAs/GaSb typ II suprlattics L.L. Li 1, W. Xu 1, 3, Z. Zg 1, ad Y.L. Si 1 Ky Laboratory of Matrials Pysics, Istitut of Solid

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

07 - SEQUENCES AND SERIES Page 1 ( Answers at he end of all questions ) b, z = n

07 - SEQUENCES AND SERIES Page 1 ( Answers at he end of all questions ) b, z = n 07 - SEQUENCES AND SERIES Pag ( Aswrs at h d of all qustios ) ( ) If = a, y = b, z = c, whr a, b, c ar i A.P. ad = 0 = 0 = 0 l a l

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

EE 232 Lightwave Devices Lecture 3: Basic Semiconductor Physics and Optical Processes. Optical Properties of Semiconductors

EE 232 Lightwave Devices Lecture 3: Basic Semiconductor Physics and Optical Processes. Optical Properties of Semiconductors 3 Lightwav Dvics Lctur 3: Basic Smicoductor Physics ad Optical Procsss Istructor: Mig C. Wu Uivrsity of Califoria, Brly lctrical girig ad Computr Scics Dpt. 3 Lctur 3- Optical Proprtis of Smicoductors

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

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

Solution to 1223 The Evil Warden.

Solution to 1223 The Evil Warden. Solutio to 1 Th Evil Ward. This is o of thos vry rar PoWs (I caot thik of aothr cas) that o o solvd. About 10 of you submittd th basic approach, which givs a probability of 47%. I was shockd wh I foud

More information

Option 3. b) xe dx = and therefore the series is convergent. 12 a) Divergent b) Convergent Proof 15 For. p = 1 1so the series diverges.

Option 3. b) xe dx = and therefore the series is convergent. 12 a) Divergent b) Convergent Proof 15 For. p = 1 1so the series diverges. Optio Chaptr Ercis. Covrgs to Covrgs to Covrgs to Divrgs Covrgs to Covrgs to Divrgs 8 Divrgs Covrgs to Covrgs to Divrgs Covrgs to Covrgs to Covrgs to Covrgs to 8 Proof Covrgs to π l 8 l a b Divrgt π Divrgt

More information

Washington State University

Washington State University he 3 Ktics ad Ractor Dsig Sprg, 00 Washgto Stat Uivrsity Dpartmt of hmical Egrg Richard L. Zollars Exam # You will hav o hour (60 muts) to complt this xam which cosists of four (4) problms. You may us

More information

MILLIKAN OIL DROP EXPERIMENT

MILLIKAN OIL DROP EXPERIMENT 11 Oct 18 Millika.1 MILLIKAN OIL DROP EXPERIMENT This xprimt is dsigd to show th quatizatio of lctric charg ad allow dtrmiatio of th lmtary charg,. As i Millika s origial xprimt, oil drops ar sprayd ito

More information

University of Washington Department of Chemistry Chemistry 453 Winter Quarter 2014 Lecture 20: Transition State Theory. ERD: 25.14

University of Washington Department of Chemistry Chemistry 453 Winter Quarter 2014 Lecture 20: Transition State Theory. ERD: 25.14 Univrsity of Wasinton Dpartmnt of Cmistry Cmistry 453 Wintr Quartr 04 Lctur 0: Transition Stat Tory. ERD: 5.4. Transition Stat Tory Transition Stat Tory (TST) or ctivatd Complx Tory (CT) is a raction mcanism

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

Digital Signal Processing, Fall 2006

Digital Signal Processing, Fall 2006 Digital Sigal Procssig, Fall 6 Lctur 9: Th Discrt Fourir Trasfor Zhg-Hua Ta Dpartt of Elctroic Systs Aalborg Uivrsity, Dar zt@o.aau.d Digital Sigal Procssig, I, Zhg-Hua Ta, 6 Cours at a glac MM Discrt-ti

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

Worksheet: Taylor Series, Lagrange Error Bound ilearnmath.net

Worksheet: Taylor Series, Lagrange Error Bound ilearnmath.net Taylor s Thorm & Lagrag Error Bouds Actual Error This is th ral amout o rror, ot th rror boud (worst cas scario). It is th dirc btw th actual () ad th polyomial. Stps:. Plug -valu ito () to gt a valu.

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

Discrete Fourier Transform. Nuno Vasconcelos UCSD

Discrete Fourier Transform. Nuno Vasconcelos UCSD Discrt Fourir Trasform uo Vascoclos UCSD Liar Shift Ivariat (LSI) systms o of th most importat cocpts i liar systms thory is that of a LSI systm Dfiitio: a systm T that maps [ ito y[ is LSI if ad oly if

More information

Topological Insulators in 2D and 3D

Topological Insulators in 2D and 3D Topological Isulators i D ad 3D 0. Elctric polarizatio, Chr Numbr, Itgr Quatum Hall Effct I. Graph - Halda modl - Tim rvrsal symmtry ad Kramrs thorm II. D quatum spi Hall isulator - Z topological ivariat

More information

Part B: Transform Methods. Professor E. Ambikairajah UNSW, Australia

Part B: Transform Methods. Professor E. Ambikairajah UNSW, Australia Part B: Trasform Mthods Chaptr 3: Discrt-Tim Fourir Trasform (DTFT) 3. Discrt Tim Fourir Trasform (DTFT) 3. Proprtis of DTFT 3.3 Discrt Fourir Trasform (DFT) 3.4 Paddig with Zros ad frqucy Rsolutio 3.5

More information

Ideal crystal : Regulary ordered point masses connected via harmonic springs

Ideal crystal : Regulary ordered point masses connected via harmonic springs Statistical thrmodyamics of crystals Mooatomic crystal Idal crystal : Rgulary ordrd poit masss coctd via harmoic sprigs Itratomic itractios Rprstd by th lattic forc-costat quivalt atom positios miima o

More information

dy 1. If fx ( ) is continuous at x = 3, then 13. If y x ) for x 0, then f (g(x)) = g (f (x)) when x = a. ½ b. ½ c. 1 b. 4x a. 3 b. 3 c.

dy 1. If fx ( ) is continuous at x = 3, then 13. If y x ) for x 0, then f (g(x)) = g (f (x)) when x = a. ½ b. ½ c. 1 b. 4x a. 3 b. 3 c. AP CALCULUS BC SUMMER ASSIGNMENT DO NOT SHOW YOUR WORK ON THIS! Complt ts problms during t last two wks of August. SHOW ALL WORK. Know ow to do ALL of ts problms, so do tm wll. Itms markd wit a * dnot

More information

Atom as a Dressed Nucleus

Atom as a Dressed Nucleus tom as a Drssd Nuclus Vladimir Kalitviaski Comissariat à l Ergi tomiqu (CE), Grobl 38054, Frac vladimir.kalitviaski@waadoo.fr W show that th lctrostatic pottial of a atomic uclus "s" by a fast chargd projctil

More information

Chp6. pn Junction Diode: I-V Characteristics I

Chp6. pn Junction Diode: I-V Characteristics I 147 C6. uctio Diod: I-V Caractristics I 6.1. THE IDEAL DIODE EQUATION 6.1.1. Qualitativ Drivatio 148 Figur rfrc: Smicoductor Dvic Fudamtals Robrt F. Pirrt, Addiso-Wsly Publicig Comay 149 Figur 6.1 juctio

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

NET/JRF, GATE, IIT JAM, JEST, TIFR

NET/JRF, GATE, IIT JAM, JEST, TIFR Istitut for NET/JRF, GATE, IIT JAM, JEST, TIFR ad GRE i PHYSICAL SCIENCES Mathmatical Physics JEST-6 Q. Giv th coditio φ, th solutio of th quatio ψ φ φ is giv by k. kφ kφ lφ kφ lφ (a) ψ (b) ψ kφ (c) ψ

More information

PHYS-333: Problem set #2 Solutions

PHYS-333: Problem set #2 Solutions PHYS-333: Problm st #2 Solutions Vrsion of March 5, 2016. 1. Visual binary 15 points): Ovr a priod of 10 yars, two stars sparatd by an angl of 1 arcsc ar obsrvd to mov through a full circl about a point

More information

H2 Mathematics Arithmetic & Geometric Series ( )

H2 Mathematics Arithmetic & Geometric Series ( ) H Mathmatics Arithmtic & Gomtric Sris (08 09) Basic Mastry Qustios Arithmtic Progrssio ad Sris. Th rth trm of a squc is 4r 7. (i) Stat th first four trms ad th 0th trm. (ii) Show that th squc is a arithmtic

More information

Discrete Fourier Transform. Discrete Fourier Transform. Discrete Fourier Transform. Discrete Fourier Transform. Discrete Fourier Transform

Discrete Fourier Transform. Discrete Fourier Transform. Discrete Fourier Transform. Discrete Fourier Transform. Discrete Fourier Transform Discrt Fourir Trasform Dfiitio - T simplst rlatio btw a lt- squc x dfid for ω ad its DTFT X ( ) is ω obtaid by uiformly sampli X ( ) o t ω-axis btw ω < at ω From t dfiitio of t DTFT w tus av X X( ω ) ω

More information

Class #24 Monday, April 16, φ φ φ

Class #24 Monday, April 16, φ φ φ lass #4 Moday, April 6, 08 haptr 3: Partial Diffrtial Equatios (PDE s First of all, this sctio is vry, vry difficult. But it s also supr cool. PDE s thr is mor tha o idpdt variabl. Exampl: φ φ φ φ = 0

More information

Narayana IIT Academy

Narayana IIT Academy INDIA Sc: LT-IIT-SPARK Dat: 9--8 6_P Max.Mars: 86 KEY SHEET PHYSIS A 5 D 6 7 A,B 8 B,D 9 A,B A,,D A,B, A,B B, A,B 5 A 6 D 7 8 A HEMISTRY 9 A B D B B 5 A,B,,D 6 A,,D 7 B,,D 8 A,B,,D 9 A,B, A,B, A,B,,D A,B,

More information

PHYS-3301 Lecture 9. CHAPTER 5 Wave Properties of Matter and Quantum Mechanics I. 5.3: Electron Scattering. Bohr s Quantization Condition

PHYS-3301 Lecture 9. CHAPTER 5 Wave Properties of Matter and Quantum Mechanics I. 5.3: Electron Scattering. Bohr s Quantization Condition CHAPTER 5 Wave Properties of Matter ad Quatum Mecaics I PHYS-3301 Lecture 9 Sep. 5, 018 5.1 X-Ray Scatterig 5. De Broglie Waves 5.3 Electro Scatterig 5.4 Wave Motio 5.5 Waves or Particles? 5.6 Ucertaity

More information

Lectures 9 IIR Systems: First Order System

Lectures 9 IIR Systems: First Order System EE3054 Sigals ad Systms Lcturs 9 IIR Systms: First Ordr Systm Yao Wag Polytchic Uivrsity Som slids icludd ar xtractd from lctur prstatios prpard by McCllla ad Schafr Lics Ifo for SPFirst Slids This work

More information

DTFT Properties. Example - Determine the DTFT Y ( e ) of n. Let. We can therefore write. From Table 3.1, the DTFT of x[n] is given by 1

DTFT Properties. Example - Determine the DTFT Y ( e ) of n. Let. We can therefore write. From Table 3.1, the DTFT of x[n] is given by 1 DTFT Proprtis Exampl - Dtrmi th DTFT Y of y α µ, α < Lt x α µ, α < W ca thrfor writ y x x From Tabl 3., th DTFT of x is giv by ω X ω α ω Copyright, S. K. Mitra Copyright, S. K. Mitra DTFT Proprtis DTFT

More information

Statistics 3858 : Likelihood Ratio for Exponential Distribution

Statistics 3858 : Likelihood Ratio for Exponential Distribution Statistics 3858 : Liklihood Ratio for Expotial Distributio I ths two xampl th rjctio rjctio rgio is of th form {x : 2 log (Λ(x)) > c} for a appropriat costat c. For a siz α tst, usig Thorm 9.5A w obtai

More information

Introduction to Quantum Information Processing. Overview. A classical randomised algorithm. q 3,3 00 0,0. p 0,0. Lecture 10.

Introduction to Quantum Information Processing. Overview. A classical randomised algorithm. q 3,3 00 0,0. p 0,0. Lecture 10. Itroductio to Quatum Iformatio Procssig Lctur Michl Mosca Ovrviw! Classical Radomizd vs. Quatum Computig! Dutsch-Jozsa ad Brsti- Vazirai algorithms! Th quatum Fourir trasform ad phas stimatio A classical

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

PHYS-3301 Lecture 7. CHAPTER 4 Structure of the Atom. Rutherford Scattering. Sep. 18, 2018

PHYS-3301 Lecture 7. CHAPTER 4 Structure of the Atom. Rutherford Scattering. Sep. 18, 2018 CHAPTER 4 Structure of the Atom PHYS-3301 Lecture 7 4.1 The Atomic Models of Thomso ad Rutherford 4.2 Rutherford Scatterig 4.3 The Classic Atomic Model 4.4 The Bohr Model of the Hydroge Atom 4.5 Successes

More information

2.29 Numerical Fluid Mechanics Spring 2015 Lecture 12

2.29 Numerical Fluid Mechanics Spring 2015 Lecture 12 REVIEW Lctur 11: Numrical Fluid Mchaics Sprig 2015 Lctur 12 Fiit Diffrcs basd Polyomial approximatios Obtai polyomial (i gral u-qually spacd), th diffrtiat as dd Nwto s itrpolatig polyomial formulas Triagular

More information

The Quantum Efficiency and Thermal Emittance of Metal Cathodes

The Quantum Efficiency and Thermal Emittance of Metal Cathodes T Quantum fficincy and Trmal mittanc of Mtal Catods David H. Dowll Tory Sminar Jun, 6 I. Introduction II. Q and Trmal mittanc Tory III. Ral World Issus Surfac Rougnss Masurmnts Diamond Turning vs. Polising

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

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

ENGG 1203 Tutorial. Difference Equations. Find the Pole(s) Finding Equations and Poles

ENGG 1203 Tutorial. Difference Equations. Find the Pole(s) Finding Equations and Poles ENGG 03 Tutoial Systms ad Cotol 9 Apil Laig Obctivs Z tasfom Complx pols Fdbac cotol systms Ac: MIT OCW 60, 6003 Diffc Equatios Cosid th systm pstd by th followig diffc quatio y[ ] x[ ] (5y[ ] 3y[ ]) wh

More information

Quantum Mechanics & Spectroscopy Prof. Jason Goodpaster. Problem Set #2 ANSWER KEY (5 questions, 10 points)

Quantum Mechanics & Spectroscopy Prof. Jason Goodpaster. Problem Set #2 ANSWER KEY (5 questions, 10 points) Chm 5 Problm St # ANSWER KEY 5 qustios, poits Qutum Mchics & Spctroscopy Prof. Jso Goodpstr Du ridy, b. 6 S th lst pgs for possibly usful costts, qutios d itgrls. Ths will lso b icludd o our futur ms..

More information

How many neutrino species?

How many neutrino species? ow may utrio scis? Two mthods for dtrmii it lium abudac i uivrs At a collidr umbr of utrio scis Exasio of th uivrs is ovrd by th Fridma quatio R R 8G tot Kc R Whr: :ubblcostat G :Gravitatioal costat 6.

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

Circular Array of Tapered Nylon Rod Antennas: A Computational Study

Circular Array of Tapered Nylon Rod Antennas: A Computational Study tratioal Joural of Elctroics ad Commuicatio Egirig. SSN 974-266 Volum 4, Numbr (2), pp.3-38 tratioal Rsarch Publicatio Hous http://www.irphous.com Circular Array of Taprd Nylo Rod Atas: A Computatioal

More information

Time Dependent Solutions: Propagators and Representations

Time Dependent Solutions: Propagators and Representations Tim Dpdt Solutios: Propagators ad Rprstatios Michal Fowlr, UVa 1/3/6 Itroductio W v spt most of th cours so far coctratig o th igstats of th amiltoia, stats whos tim dpdc is mrly a chagig phas W did mtio

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

Scattering Parameters. Scattering Parameters

Scattering Parameters. Scattering Parameters Motivatio cattrig Paramtrs Difficult to implmt op ad short circuit coditios i high frqucis masurmts du to parasitic s ad Cs Pottial stability problms for activ dvics wh masurd i oopratig coditios Difficult

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

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

Estimation of the two-photon QED background in Belle II

Estimation of the two-photon QED background in Belle II Estimation of th two-photon QED background in Bll II Elna Ndlkovska, Christian Kisling Max-Planck Institut for physics, Munich Upgrad to th Bll II dtctor Expctd background at Bll II QED xprimnts prformd

More information

Time : 1 hr. Test Paper 08 Date 04/01/15 Batch - R Marks : 120

Time : 1 hr. Test Paper 08 Date 04/01/15 Batch - R Marks : 120 Tim : hr. Tst Papr 8 D 4//5 Bch - R Marks : SINGLE CORRECT CHOICE TYPE [4, ]. If th compl umbr z sisfis th coditio z 3, th th last valu of z is qual to : z (A) 5/3 (B) 8/3 (C) /3 (D) o of ths 5 4. Th itgral,

More information

A Simple Proof that e is Irrational

A Simple Proof that e is Irrational Two of th most bautiful ad sigificat umbrs i mathmatics ar π ad. π (approximatly qual to 3.459) rprsts th ratio of th circumfrc of a circl to its diamtr. (approximatly qual to.788) is th bas of th atural

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

PHY 410. Final Examination, Spring May 4, 2009 (5:45-7:45 p.m.)

PHY 410. Final Examination, Spring May 4, 2009 (5:45-7:45 p.m.) PHY ina amination, Spring 9 May, 9 5:5-7:5 p.m. PLAS WAIT UTIL YOU AR TOLD TO BGI TH XAM. Wi waiting, carfuy fi in t information rqustd bow Your am: Your Studnt umbr: DO OT TUR THIS PAG UTIL TH XAM STARTS

More information

1 of 42. Abbreviated title: [SAP-SVT-Nmsm-g & 137] - Updated on 31 July, 09. Shankar V.Narayanan

1 of 42. Abbreviated title: [SAP-SVT-Nmsm-g & 137]  - Updated on 31 July, 09. Shankar V.Narayanan 1 of 4 ONE EQUATION ad FOUR Subatomic Particls ad thir FOUR Itractios icludig (g &17) factors with Spac Vortx Thory (A No matrial shll modl) (Part 1 of ) (Th cotts of this txt ar th sam as i Subatomic

More information

Electromagnetic radiation and steady states of hydrogen atom

Electromagnetic radiation and steady states of hydrogen atom Elctromagtic radiatio ad stady stats of hydrog atom Jiaomig Luo Egirig Rsarch Ctr i Biomatrials, Sichua Uivrsity, 9# Wagjiag Road, Chgdu, Chia, 610064 Abstract. Elctromagtic phoma i hydrog atom ar cotrolld

More information

Chapter 11 Solutions ( ) 1. The wavelength of the peak is. 2. The temperature is found with. 3. The power is. 4. a) The power is

Chapter 11 Solutions ( ) 1. The wavelength of the peak is. 2. The temperature is found with. 3. The power is. 4. a) The power is Chapt Solutios. Th wavlgth of th pak is pic 3.898 K T 3.898 K 373K 885 This cospods to ifad adiatio.. Th tpatu is foud with 3.898 K pic T 3 9.898 K 50 T T 5773K 3. Th pow is 4 4 ( 0 ) P σ A T T ( ) ( )

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

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

S- AND P-POLARIZED REFLECTIVITIES OF EXPLOSIVELY DRIVEN STRONGLY NON-IDEAL XENON PLASMA

S- AND P-POLARIZED REFLECTIVITIES OF EXPLOSIVELY DRIVEN STRONGLY NON-IDEAL XENON PLASMA S- AND P-POLARIZED REFLECTIVITIES OF EXPLOSIVELY DRIVEN STRONGLY NON-IDEAL XENON PLASMA Zaporozhts Yu.B.*, Mitsv V.B., Gryazov V.K., Riholz H., Röpk G. 3, Fortov V.E. 4 Istitut of Problms of Chmical Physics

More information

Chapter 2 Infinite Series Page 1 of 11. Chapter 2 : Infinite Series

Chapter 2 Infinite Series Page 1 of 11. Chapter 2 : Infinite Series Chatr Ifiit Sris Pag of Sctio F Itgral Tst Chatr : Ifiit Sris By th d of this sctio you will b abl to valuat imror itgrals tst a sris for covrgc by alyig th itgral tst aly th itgral tst to rov th -sris

More information

Trigonometric functions

Trigonometric functions Robrto s Nots on Diffrntial Calculus Captr 5: Drivativs of transcndntal functions Sction 5 Drivativs of Trigonomtric functions Wat you nd to know alrady: Basic trigonomtric limits, t dfinition of drivativ,

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

5.80 Small-Molecule Spectroscopy and Dynamics

5.80 Small-Molecule Spectroscopy and Dynamics MIT OpnCoursWar http://ocw.mit.du 5.80 Small-Molcul Spctroscopy and Dynamics Fall 008 For information about citing ths matrials or our Trms of Us, visit: http://ocw.mit.du/trms. Lctur # 3 Supplmnt Contnts

More information

Chapter Five. More Dimensions. is simply the set of all ordered n-tuples of real numbers x = ( x 1

Chapter Five. More Dimensions. is simply the set of all ordered n-tuples of real numbers x = ( x 1 Chatr Fiv Mor Dimsios 51 Th Sac R W ar ow rard to mov o to sacs of dimsio gratr tha thr Ths sacs ar a straightforward gralizatio of our Euclida sac of thr dimsios Lt b a ositiv itgr Th -dimsioal Euclida

More information

CIVE322 BASIC HYDROLOGY Hydrologic Science and Engineering Civil and Environmental Engineering Department Fort Collins, CO (970)

CIVE322 BASIC HYDROLOGY Hydrologic Science and Engineering Civil and Environmental Engineering Department Fort Collins, CO (970) CVE322 BASC HYDROLOGY Hydrologic Scic ad Egirig Civil ad Evirotal Egirig Dpartt Fort Collis, CO 80523-1372 (970 491-7621 MDERM EXAM 1 NO. 1 Moday, Octobr 3, 2016 8:00-8:50 AM Haod Auditoriu You ay ot cosult

More information

Discrete Fourier Transform (DFT)

Discrete Fourier Transform (DFT) Discrt Fourir Trasorm DFT Major: All Egirig Majors Authors: Duc guy http://umricalmthods.g.us.du umrical Mthods or STEM udrgraduats 8/3/29 http://umricalmthods.g.us.du Discrt Fourir Trasorm Rcalld th xpotial

More information