(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)

Size: px
Start display at page:

Download "(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)"

Transcription

1 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) Lt s first considr (1) intractions of chargd particls with mattr via m. Litratur: B. Rossi High Enrgy Particls, Prntic Hall, Inc., Englwood Cliffs, NJ, 195 J.D. Jackson, Classical Elctrodynamics, Chaptr 13 Print: rv passag particls mattr.pdf

2 Gnral Disposition Swift particl with charg z and mass M (. g. m, p, d, a...) with E = gmc and p = gbmc collids with atomic lctron of mass m = m and charg (-). Elctrons ar in atoms with Z, and A. Enrgy losss of particl with mass M ar from th collisions with atomic lctrons. In many cass binding nrgy of lctrons in atoms can b nglctd for nrgtic collisions "scattring on fr lctrons" Enrgy losss of all particls with M m ( mp,, K, p, d, a...) can b dscribd by gnral law (from Ruthrford scattring) with M as a paramtr (+spin) + - Enrgy losss by or particls ar tratd diffrntly di to M = m Elctromagntic intractions of nutal particls ar not zro, but vry small (.g. nutrons). Elastic M on m via Coulomb scattring Ruthrford scattring f-la

3 Enrgy loss X-sction for scattring particls m 1 and m T = mv nrgy transfrrd in Lab from particl 1 to particl = nrgy lost by particl 1 in Lab v 1 = v sin LL1 (17.5) m1 + m Q d =, Î é0, E ù ë max û mv ds p E = m 3 ø 4mm c æ Q ö cos c ds = p ç dc çèmv sin c 1 max E 1 Lab ( m1 + m) m = v m Ruthrford scattring for Ur () ds µ d c sin Q = r 1 is for Coulomb (= atomic) fild. Compar with ds d = const for.g. na low-nrgy scattring 1

4 Scattring of particl with mass m and charg z on lctrons in mattr (lctrons ar in atoms with Z and A) [4] B. Rossi High Enrgy Particls, Prntic Hall, Inc., Englwood Cliffs, NJ, 195!

5 Enrgtic knock out of lctrons ( rays)

6 T Enrgy loss X-sction for scattring particls m 1 and m v = = mv nrgy transfrrd in Lab from particl 1 to particl = nrgy lost by particl 1 in Lab 1 = v sin LL1 (17.5) m1 + m Q d =, Î é0, E ù ë max û mv ds p E = m 3 ø 4mm c æ Q ö cos c ds = p ç dc çèmv sin c 1 max E 1 Lab ( m1 + m) m = v m Ruthrford scattring Ur () c sin Q = r ds 1 ds 1 µ or µ d dt T this is non - rlativistic tratmnt, T kintic nrgy transfrrd to lctron = nrgy loss by incidnt particl [Rmmbr t =- mt is invariant]

7 dn - probabilty distribution function (pdf) for charg particl with vlocity dtdx passing th layr of thicknss dx [ dx] usually xprssd in units g cm ( dx = r dl) b A K 4p whr Nrmc MV = = A A gcm é T ù FT ( ) = 1 -b for incidnt spin 0 particl (Bhabha) ê T ú ë max û é 1 for spin incidnt T 1æ T ö ù FT ( ) = 1 b - + T (Bhabha+Massy+Corbr) max ê ç è Mc ø ë E + ú û é æ T öæ 1 T ö ù 1 T FT ( ) = 1 b 1 æ ö æ 1 T ö ç çè T 1 ç max øè 3T C ø 3 + ê ç èe + Mc ø çè T C ø ë ú û for incidnt spin 1 particl (Massy+Corbr+Oppnhimr+...) rlativistic formula FT ( ) includs QFT spin tratmnt of colliding particls T C for A= 1g mol b r Mc m v = ; c = = 4p mc 0.8fm classical lctron radius; z - charg of particl

8 rlativistic formula from your HW sinc mm 1 and whn g is not vry larg th Tmax mcb g dn and ar ~"indpndnt" on mass M (but function of b= pc E or g= E M) dtdx - For incidnt (Møllr) for dn 1 Zé é 1 1 T ( T ) ù E ù KZê - E + E ú = K - = ë û E dtdx A êt( T) A ë E - E ú û ( E -T) T + For incidnt (Bhabha) for E mc é 1 T ( T ) ù dn KZê - E + E ú = ë û é1 T ( T ) ù dtdx A ê - E + E ú E ( E -T) T ë û E mc additional trm du to possibl positron and lctron rcoils

9 Exrcis: What is Tmax if incidnt particl is -? T max mc bg mc bg Ebg æ 1ö = = = = E 1 - = 1 g m ( m) 1+ g 1+ g ç è g + + ø M M T kin _ inc - - Howvr, in scattring lctrons ar not distinguishabl T max = E F-la for positrons is tratd as T = E as wll!!! max Mc If T T max and T T C = all abov f-las ar transform m dn K Z 1 1 to Ruthrford's formula: = z dtdx A b T 1 not whn T 0 T du to long-rang of -m forc

10 T max de æ d N ö - ( T > ) = T dt ; I (avrag ionozation potntial dx ò ç çèdtdx ø as minimum transfr nrgy) Bth Bloch formula: calld lctronic stopping powr for M>m particls K MV éde ù MV ê ú = A g cm ëdx û g cm accuracy of B-B f-la is about 1% hr 0.3 ê ú in th "usful" nrgy rang de For practical purposs in a givn matrial is function of only bg; dx de p for all havy particls sam ( bg) can b usd; bg = dx Mc

11

12

13 Stopping powr and Rang DE= x ò x1 de dx dx E E dx de D x= ò de = ò de æ de ö E1 E1 ç èdx ø E1 x1 x = E E = E -DE dx Rrang ( )( E) 0 de = ò æ de ö E ç èdx ø

14 Stopping powr Rangs

15 Stopping Powr and Rang Tabls for Elctrons, Protons, and Hlium Ions: (a) (b)

16 Avrag ionization potntial I = man xcitation nrgy is an important non-trivial paramtr that is dtmind xprimntally compar with known I=13.6 V for hydrogn

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

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

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

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

Lecture 2. Interaction of Radiation with Matter

Lecture 2. Interaction of Radiation with Matter Lctur Intraction of Radiation with Mattr Dats 14.10. Vorlsung 1 T.Stockmanns 1.10. Vorlsung J.Ritman 8.10. Vorlsung 3 J.Ritman 04.11. Vorlsung 4 J.Ritman 11.11. Vorlsung 5 J.Ritman 18.11. Vorlsung 6 J.

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

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

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

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

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

The United States Nuclear Regulatory Commission and Duke University Present: Regulatory and Radiation Protection Issues in Radionuclide Therapy

The United States Nuclear Regulatory Commission and Duke University Present: Regulatory and Radiation Protection Issues in Radionuclide Therapy Th Unitd Stats Nuclar Rgulatory Commission and Duk Univrsity Prsnt: Rgulatory and Radiation Protction Issus in Radionuclid Thrapy Copyright 008 Duk Radiation Safty and Duk Univrsity. All Rights Rsrvd.

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

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

Forces. Quantum ElectroDynamics. α = = We have now: W hav now: Forcs Considrd th gnral proprtis of forcs mdiatd by xchang (Yukawa potntial); Examind consrvation laws which ar obyd by (som) forcs. W will nxt look at thr forcs in mor dtail: Elctromagntic

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

Interaction of particles with matter

Interaction of particles with matter Introduction to Elmntary Particl Physics. Not 1 Pag 1 of 15 Intraction of particls with mattr 1. Particls and intractions. Wak intractions (nutrinos) 3. Elctromagntic intractions (chargd particls) 3.1.

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

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

Maxwellian Collisions

Maxwellian Collisions Maxwllian Collisions Maxwll ralizd arly on that th particular typ of collision in which th cross-sction varis at Q rs 1/g offrs drastic siplifications. Intrstingly, this bhavior is physically corrct for

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

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 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

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

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

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

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

September 23, Honors Chem Atomic structure.notebook. Atomic Structure Atomic Structur Topics covrd Atomic structur Subatomic particls Atomic numbr Mass numbr Charg Cations Anions Isotops Avrag atomic mass Practic qustions atomic structur Sp 27 8:16 PM 1 Powr Standards/ Larning

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

Spring 2012, P627, YK Friday, January 27, 2012

Spring 2012, P627, YK Friday, January 27, 2012 7 Spring 1, P67, YK Friday, January 7, 1 Topic Software Talk date Kubra PC+VM Rachel Dark Matter PC+VM Joel Mac+? Chris PC+VM Kyle Linux +VM Possible project talk dates: pril 18,,3,5,7 Projects: Proton

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

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

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

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

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

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

Lecture Outline. Skin Depth Power Flow 8/7/2018. EE 4347 Applied Electromagnetics. Topic 3e

Lecture Outline. Skin Depth Power Flow 8/7/2018. EE 4347 Applied Electromagnetics. Topic 3e 8/7/018 Cours Instructor Dr. Raymond C. Rumpf Offic: A 337 Phon: (915) 747 6958 E Mail: rcrumpf@utp.du EE 4347 Applid Elctromagntics Topic 3 Skin Dpth & Powr Flow Skin Dpth Ths & Powr nots Flow may contain

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

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

Nuclear reactions The chain reaction

Nuclear reactions The chain reaction Nuclar ractions Th chain raction Nuclar ractions Th chain raction For powr applications want a slf-sustaind chain raction. Natural U: 0.7% of 235 U and 99.3% of 238 U Natural U: 0.7% of 235 U and 99.3%

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

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

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

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

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

Chapter 8: Electron Configurations and Periodicity

Chapter 8: Electron Configurations and Periodicity Elctron Spin & th Pauli Exclusion Principl Chaptr 8: Elctron Configurations and Priodicity 3 quantum numbrs (n, l, ml) dfin th nrgy, siz, shap, and spatial orintation of ach atomic orbital. To xplain how

More information

Einstein Equations for Tetrad Fields

Einstein Equations for Tetrad Fields Apiron, Vol 13, No, Octobr 006 6 Einstin Equations for Ttrad Filds Ali Rıza ŞAHİN, R T L Istanbul (Turky) Evry mtric tnsor can b xprssd by th innr product of ttrad filds W prov that Einstin quations for

More information

Neutrino Probes of Dark Energy and Dark Matter

Neutrino Probes of Dark Energy and Dark Matter SNOWPAC@Snowbird March 25, 2010 Nutrino Probs of Dark Enrgy and Dark Mattr Shin ichiro Ando California Institut of Tchnology Dark Enrgy and Dark Mattr 2.0 1.5 1.0 No Big Bang SN Most of th nrgy in th Univrs

More information

1.2 Faraday s law A changing magnetic field induces an electric field. Their relation is given by:

1.2 Faraday s law A changing magnetic field induces an electric field. Their relation is given by: Elctromagntic Induction. Lorntz forc on moving charg Point charg moving at vlocity v, F qv B () For a sction of lctric currnt I in a thin wir dl is Idl, th forc is df Idl B () Elctromotiv forc f s any

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

Slowing-down processes, energy deposition, sputtering and desorption in ion and electron interactions with solids

Slowing-down processes, energy deposition, sputtering and desorption in ion and electron interactions with solids Slowing-down procsss, nrgy dposition, sputtring and dsorption in ion and lctron intractions with solids J. Schou Risø National Laboratory, DK-4000 Roskild, Dnmark Abstract Th slowing-down procsss of ions

More information

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

Neutrinos are chargeless, nearly massless particles Most abundant particle in the Universe Interact with matter via weak nuclear force By Wndi Wamlr Nutrinos ar charglss, narly masslss articls Most abundant articl in th Univrs Intract with mattr via wak nuclar forc Narly transarnt to mattr Only known ty of articl that can sca from th

More information

Part 7: Capacitance And Capacitors

Part 7: Capacitance And Capacitors Part 7: apacitanc And apacitors 7. Elctric harg And Elctric Filds onsidr a pair of flat, conducting plats, arrangd paralll to ach othr (as in figur 7.) and sparatd by an insulator, which may simply b air.

More information

Pion condensation with neutrinos

Pion condensation with neutrinos Pion condnsation with nutrinos Or how dos QCD bhav undr high dnsitis of lctron/muon nutrinos Harmn Warringa, Goth Univrsität, Frankfurt Basd on work don with Hiroaki Abuki and Tomas Braunr arxiv:0901.2477

More information

Slowing-down processes, energy deposition, sputtering and desorption in ion and electron interactions with solids.

Slowing-down processes, energy deposition, sputtering and desorption in ion and electron interactions with solids. Slowing-down procsss, nrgy dposition, sputtring and dsorption in ion and lctron intractions with solids. Jørgn Schou Dpartmnt of Optics and Plasma Rsarch, Risø National Laboratory, DK-4000 Roskild, Dnmark.

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

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

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

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

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

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

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

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

Particle Physics. Dr M.A. Thomson. e + γ. 1 q 2. e - Part II, Lent Term 2004 HANDOUT II. Dr M.A. Thomson Lent 2004

Particle Physics. Dr M.A. Thomson. e + γ. 1 q 2. e - Part II, Lent Term 2004 HANDOUT II. Dr M.A. Thomson Lent 2004 Particl Physics Dr M.A. Thomson µ q 2 µ Part II, Lnt Trm 2004 HANDOUT II Dr M.A. Thomson Lnt 2004 Quantum Elctrodynamics 2 QUANTUM ELECTRODYNAMICS: is th quantum thory of th lctromagntic intraction. CLASSICAL

More information

Chapter 7b Electron Spin and Spin- Orbit Coupling

Chapter 7b Electron Spin and Spin- Orbit Coupling Wintr 3 Chm 356: Introductory Quantum Mchanics Chaptr 7b Elctron Spin and Spin- Orbit Coupling... 96 H- atom in a Magntic Fild: Elctron Spin... 96 Total Angular Momntum... 3 Chaptr 7b Elctron Spin and

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

F O R SOCI AL WORK RESE ARCH

F O R SOCI AL WORK RESE ARCH 7 TH EUROPE AN CONFERENCE F O R SOCI AL WORK RESE ARCH C h a l l e n g e s i n s o c i a l w o r k r e s e a r c h c o n f l i c t s, b a r r i e r s a n d p o s s i b i l i t i e s i n r e l a t i o n

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

Constants and Conversions:

Constants and Conversions: EXAM INFORMATION Radial Distribution Function: P 2 ( r) RDF( r) Br R( r ) 2, B is th normalization constant. Ordr of Orbital Enrgis: Homonuclar Diatomic Molculs * * * * g1s u1s g 2s u 2s u 2 p g 2 p g

More information

Cosmology and particle physics

Cosmology and particle physics Cosmology and particl physics Lctur nots Timm Wras Lctur 8 Th thrmal univrs - part IV In this lctur w discuss th Boltzmann quation that allows on to dscrib th volution of procsss in our univrs that ar

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

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

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

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

0 +1e Radionuclides - can spontaneously emit particles and radiation which can be expressed by a nuclear equation. Radioactivity Radionuclids - can spontanously mit particls and radiation which can b xprssd by a nuclar quation. Spontanous Emission: Mass and charg ar consrvd. 4 2α -β Alpha mission Bta mission 238 92U

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

Engineering 323 Beautiful HW #13 Page 1 of 6 Brown Problem 5-12

Engineering 323 Beautiful HW #13 Page 1 of 6 Brown Problem 5-12 Enginring Bautiful HW #1 Pag 1 of 6 5.1 Two componnts of a minicomputr hav th following joint pdf for thir usful liftims X and Y: = x(1+ x and y othrwis a. What is th probability that th liftim X of th

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

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

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

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

Exam 1. It is important that you clearly show your work and mark the final answer clearly, closed book, closed notes, no calculator.

Exam 1. It is important that you clearly show your work and mark the final answer clearly, closed book, closed notes, no calculator. Exam N a m : _ S O L U T I O N P U I D : I n s t r u c t i o n s : It is important that you clarly show your work and mark th final answr clarly, closd book, closd nots, no calculator. T i m : h o u r

More information

The Death of Stars - II.

The Death of Stars - II. Th Dath of Stars - II. Larning Objctivs! How can w us H-R diagrams to masur th ag of star clustrs (and hnc th ag of our Univrs)?! Why do high and low mass stars volv diffrntly? How ar havy lmnts such as

More information

Electrochemistry L E O

Electrochemistry L E O Rmmbr from CHM151 A rdox raction in on in which lctrons ar transfrrd lctrochmistry L O Rduction os lctrons xidation G R ain lctrons duction W can dtrmin which lmnt is oxidizd or rducd by assigning oxidation

More information

Antonio Pich. IFIC, CSIC Univ. Valencia.

Antonio Pich. IFIC, CSIC Univ. Valencia. Antonio Pich IFIC, CSIC Univ. Valncia Antonio.Pich@crn.ch Th Standard Modl A. Pich - CERN Summr Lcturs 2005 1. Constitunts & Intractions 2. Quarks 3. Gaug Invarianc 4. Quantum Chromodynamics 5. Elctrowak

More information

Andre Schneider P621

Andre Schneider P621 ndr Schnidr P61 Probl St #03 Novbr 6, 009 1 Srdnicki 10.3 Vrtx for L 1 = gχϕ ϕ. Th vrtx factor is ig. ϕ ig χ ϕ igur 1: ynan diagra for L 1 = gχϕ ϕ. Srdnicki 11.1 a) Dcay rat for th raction ig igur : ynan

More information

Electric (Rocket) Propulsion. EP Overview

Electric (Rocket) Propulsion. EP Overview Elctric (Rockt) Propulsion EP Ovrviw Elctric Propulsion-1 Basics Rockt Propulsion Elmnts Propllant Enrgy Sourc Storag Fd Systm sam in chmical rockts Storag Convrsion Acclrator Elctric Propulsion- 1 Elctric

More information

Self-interaction mass formula that relates all leptons and quarks to the electron

Self-interaction mass formula that relates all leptons and quarks to the electron Slf-intraction mass formula that rlats all lptons and quarks to th lctron GERALD ROSEN (a) Dpartmnt of Physics, Drxl Univrsity Philadlphia, PA 19104, USA PACS. 12.15. Ff Quark and lpton modls spcific thoris

More information

G GILMORE Practical Gamma-Ray Spectrometry (2e, Wiley, 2011) Ch 2 - Interactions of Gamma Radiation with Matter

G GILMORE Practical Gamma-Ray Spectrometry (2e, Wiley, 2011) Ch 2 - Interactions of Gamma Radiation with Matter G GILMORE Practical Gamma-Ray Spctromtry (2, Wily, 2011) Ch 2 - Intractions of Gamma Radiation with Mattr . 2 Intractions of Gamma Radiation with Mattr 2.1 INTRODUCTION In this chaptr, I will discuss th

More information

Text: WMM, Chapter 5. Sections , ,

Text: WMM, Chapter 5. Sections , , Lcturs 6 - Continuous Probabilit Distributions Tt: WMM, Chaptr 5. Sctions 6.-6.4, 6.6-6.8, 7.-7. In th prvious sction, w introduc som of th common probabilit distribution functions (PDFs) for discrt sampl

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

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

Exercise 1. Sketch the graph of the following function. (x 2

Exercise 1. Sketch the graph of the following function. (x 2 Writtn tst: Fbruary 9th, 06 Exrcis. Sktch th graph of th following function fx = x + x, spcifying: domain, possibl asymptots, monotonicity, continuity, local and global maxima or minima, and non-drivability

More information

Alpha and beta decay equation practice

Alpha and beta decay equation practice Alpha and bta dcay quation practic Introduction Alpha and bta particls may b rprsntd in quations in svral diffrnt ways. Diffrnt xam boards hav thir own prfrnc. For xampl: Alpha Bta α β alpha bta Dspit

More information

5. Equation of state for high densities

5. Equation of state for high densities 5 1 5. Equation of stat for high dnsitis Equation of stat for high dnsitis 5 Vlocity distribution of lctrons Classical thrmodynamics: 6 dimnsional phas spac: (x,y,z,px,py,pz) momntum: p = p x+p y +p z

More information

AS 5850 Finite Element Analysis

AS 5850 Finite Element Analysis AS 5850 Finit Elmnt Analysis Two-Dimnsional Linar Elasticity Instructor Prof. IIT Madras Equations of Plan Elasticity - 1 displacmnt fild strain- displacmnt rlations (infinitsimal strain) in matrix form

More information

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

A central nucleus. Protons have a positive charge Electrons have a negative charge Atomic Structur Lss than ninty yars ago scintists blivd that atoms wr tiny solid sphrs lik minut snookr balls. Sinc thn it has bn discovrd that atoms ar not compltly solid but hav innr and outr parts.

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

7.4 Potential Difference and Electric Potential

7.4 Potential Difference and Electric Potential 7.4 Potntial Diffrnc and Elctric Potntial In th prvious sction, you larnd how two paralll chargd surfacs produc a uniform lctric fild. From th dfinition of an lctric fild as a forc acting on a charg, it

More information

Lecture 24. Ideal Gas Law and Kinetic Theory

Lecture 24. Ideal Gas Law and Kinetic Theory Lecture 4 Ideal Gas Law and Kinetic Theory Today s Topics: Ideal Gas Law Kinetic Theory of Gases Phase equilibria and phase diagrams Ideal Gas Law An ideal gas is an idealized model for real gases that

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

SAFE HANDS & IIT-ian's PACE EDT-15 (JEE) SOLUTIONS

SAFE HANDS & IIT-ian's PACE EDT-15 (JEE) SOLUTIONS It is not possibl to find flu through biggr loop dirctly So w will find cofficint of mutual inductanc btwn two loops and thn find th flu through biggr loop Also rmmbr M = M ( ) ( ) EDT- (JEE) SOLUTIONS

More information

TREATMENT OF THE PLASMA NONLINEAR ABSORPTION LAW AT LINEARLY POLARIZED LASER RADIATION OF RELATIVISTIC INTENSITIES. A. G.

TREATMENT OF THE PLASMA NONLINEAR ABSORPTION LAW AT LINEARLY POLARIZED LASER RADIATION OF RELATIVISTIC INTENSITIES. A. G. Armnian Journal of Physics, 15, vol. 8, issu, pp. 64-7 TREATMENT OF THE PLASMA NONLINEAR ABSORPTION LAW AT LINEARLY POLARIZED LASER RADIATION OF RELATIVISTIC INTENSITIES A. G. Ghazaryan Cntr of Strong

More information

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

University of Illinois at Chicago Department of Physics. Thermodynamics & Statistical Mechanics Qualifying Examination Univrsity of Illinois at Chicago Dpartmnt of hysics hrmodynamics & tatistical Mchanics Qualifying Eamination January 9, 009 9.00 am 1:00 pm Full crdit can b achivd from compltly corrct answrs to 4 qustions.

More information