Constituents of the Atom

Size: px
Start display at page:

Download "Constituents of the Atom"

Transcription

1 1 Constitunts of th Atom To b know th constitunts of th atom with thir masss and chargs To b abl to calculat th spcific charg of th constitunts To b abl to xplain what isotops and ions ar Th Nuclar Modl (Also sn in GCSE Physics 1 and 2) W know from Ruthrford s xprimnt that th structur of an atom consists of positivly chargd protons and nutral nutrons in on plac calld th nuclus. Th nuclus sits in th middl of th atom and has ngativly chargd lctrons orbiting it. At GCSE w usd chargs and masss for th constitunts rlativ to ach othr, th tabl abov shows th actual chargs and masss. Constitunt (C) Mass (kg) Proton 1.6 x x Nutron x Elctron x x Almost all of th mass of th atom is in th tiny nuclus which taks up practically no spac whn compard to th siz of th atom. If w shrunk th Solar Systm so that th Sun was th siz of a gold nuclus th furthst lctron would b twic th distanc to Pluto. If th nuclus was a full stop it would b 25 m to th first lctron shll, 100 to th scond and 225 to th third. Notation (Also sn in GCSE Physics 2) W can rprsnt an atom of lmnt X in th following way: A Z X Z is th proton numbr. This is th numbr of protons in th nuclus. In an unchargd atom th numbr of lctrons orbiting th nuclus is qual to th numbr of protons. In Chmistry it is calld th atomic numbr A is th nuclon numbr. This is th total numbr of nuclons in th nuclus (protons + nutrons) which can b writtn as A = Z + N. In Chmistry it is calld th atomic mass numbr N is th nutron numbr. This is th numbr of nutrons in th nuclus. Isotops (Also sn in GCSE Physics 1 and 2) Isotops ar diffrnt forms of an lmnt. Thy always hav th sam numbr of protons but hav a diffrnt numbr of nutrons. Sinc thy hav th sam numbr of protons (and lctrons) thy bhav in th sam way chmically Chlorin If w look at Chlorin in th priodic tabl w s that it is rprsntd by 17 Cl. How can it hav nutrons? It can t! Thr ar two stabl isotops of Chlorin, 17Cl which accounts for ~75% and 17Cl which 35.5 accounts for ~25%. So th avrag of a larg amount of Chlorin atoms is 17 Cl. Spcific Spcific charg is anothr titl for th charg-mass ratio. This is a masur of th charg pr unit mass and is simply workd out by workd out by dividing th charg of a particl by its mass. You can think of it as a how much charg (in Coulombs) you gt pr kilogram of th stuff. Constitunt (C) Mass (kg) -Mass Ratio (C kg -1 ) or (C/kg) Proton 1.6 x x x x x 10 7 Nutron x x Elctron (-) 1.6 x x x x (-) 1.76 x W can s that th lctron has th highst charg-mass ratio and th nutron has th lowst. Ions (Also sn in GCSE Physics 2) An atom may gain or los lctrons. Whn this happns th atoms bcoms lctrically chargd (positivly or ngativly). W call this an ion. If th atom gains an lctron thr ar mor ngativ chargs than positiv, so th atom is a ngativ ion. Gaining on lctron would man it has an ovrall charg of -1, which actually mans -1.6 x C. Gaining two lctrons would man it has an ovrall charg of -2, which actually mans -3.2 x C. If th atom loss an lctron thr ar mor positiv chargs than ngativ, so th atom is a positiv ion. Losing on lctron would man it has an ovrall charg of +1, which actually mans +1.6 x C. Losing two lctrons would man it has an ovrall charg of +2, which actually mans +3.2 x C.

2 2 Particls and Antiparticls To know what is th diffrnc btwn particls and antiparticls To b abl to xplain what annihilation is To b abl to xplain what pair production is Antimattr British Physicist Paul Dirac prdictd a particl of qual mass to an lctron but of opposit charg (positiv). This particl is calld a positron and is th lctron s antiparticl. Evry particls has its own antiparticl. An antiparticl has th sam mass as th particl vrsion but has opposit charg. An antiproton has a ngativ charg, an antilctron has a positiv charg but an antinutron is also unchargd lik th particl vrsion. Amrican Physicist Carl Andrson obsrvd th positron in a cloud chambr, backing up Dirac s thory. Anti particls hav opposit, Numbr, Lpton Numbr and. If thy ar mad from quarks th antiparticl is mad from antiquarks Annihilation Whnvr a particl and its antiparticl mt thy annihilat ach othr. Annihilation is th procss by which mass is convrtd into nrgy, particl and antiparticl ar transformd into two photons of nrgy. Mass and nrgy ar intrchangabl and can b convrtd from on to th othr. Einstin linkd nrgy and mass with th quation: 2 E mc You can think of it lik mony; whthr you hav dollars or pounds you would still hav th sam amount of mony. So whthr you hav mass or nrgy you still hav th sam amount. Th law of consrvation of nrgy can now b rfrrd to as th consrvation of mass-nrgy. Th total mass-nrgy bfor is qual to th total mass-nrgy aftr. Photon Max Planck had th ida that light could b rlasd in chunks or packts of nrgy. Einstin namd ths wav-packts photons. Th nrgy carrid by a photon is givn by th quation: hc E hf Sinc c f w can also writ this as: E How is thr anything at all? Whn th Big Bang happnd mattr and antimattr was producd and snt out xpanding in all dirctions. A short tim aftr this thr was an imbalanc in th amount of mattr and antimattr. Sinc thr was mor mattr all th antimattr was annihilatd laving mattr to form protons, atoms and vrything around us. Pair Production Pair production is th opposit procss to annihilation, nrgy is convrtd into mass. A singl photon of nrgy is convrtd into a particl-antiparticl pair. (This happns to oby th consrvation laws) This can only happn if th photon has nough mass-nrgy to pay for th mass. Lt us imag mass and nrgy as th sam thing, if two particls ndd 10 bits and th photon had 8 bits thr is not nough for pair production to occur. If two particls ndd 10 bits to mak and th photon had 16 bits th particl-antiparticl pair is mad and th lft ovr is convrtd into thir kintic nrgy. If pair production occurs in a magntic fild th particl and antiparticl will mov in circls of opposit dirction but only if thy ar chargd. (Th dflction of chargs in magntic filds will b covrd in Unit 4: Forc on a d Particl) Pair production can occur spontanously but must occur nar a nuclus which rcoils to hlp consrv momntum. It can also b mad to happn by colliding particls. At CERN protons ar acclratd and fird into ach othr. If thy hav nough kintic nrgy whn thy collid particl-antiparticl pair may b cratd from th nrgy. Th following ar xampls of th ractions that hav occurrd: p p p p p p p p p p p p p p n n In all w can s that th consrvation laws of particl physics ar obyd.

3 3 Quarks To know what quarks ar and whr thy ar found To b abl to xplain how thy wr discovrd To know th proprtis of ach typ of quark Ruthrford Also sn in GCSE Physics 2 Ruthrford fird a bam of alpha particls at a thin gold foil. If th atom had no innr structur th alpha particls would only b dflctd by vry small angls. Som of th alpha particls wr scattrd at larg angls by th nucli of th atoms. From this Ruthrford dducd that th atom was mostly mpty spac with th majority of th mass situatd in th cntr. Atoms wr mad from smallr particls. Smallr Scattring In 1968 Physicists conductd a similar xprimnt to Ruthrford s but thy fird a bam of high nrgy lctrons at nuclons (protons and nutrons). Th rsults thy obtaind wr vry similar to Ruthrford s; som of th lctrons wr dflctd by larg angls. If th nuclons had no innr structur th lctrons would only b dflctd by small angls. Ths rsults showd that protons and nutrons wr mad of thr smallr particls, ach with a fractional charg. Quarks Ths smallr particls wr namd quarks and ar thought to b fundamntal particls (not mad of anything smallr). Thr ar six diffrnt quarks and ach on has its own antiparticl. W nd to know about th thr blow as w will b looking at how largr particls ar mad from diffrnt combinations of quarks and antiquarks. Quark Anti Quark d -⅓ +⅓ 0 d +⅓ -⅓ 0 u +⅔ +⅓ 0 u -⅔ -⅓ 0 s -⅓ +⅓ -1 s +⅓ -⅓ +1 Th othr thr ar Charm, Bottom and Top. You will not b askd about ths thr Quark No. Charmnss Bottomnss Topnss d -⅓ +⅓ u +⅔ +⅓ s -⅓ +⅓ c +⅔ +⅓ b -⅓ +⅓ t +⅔ +⅓ Th Lon Quark? Nvr! Quarks nvr appar on thir own. Th nrgy rquird to pull two quarks apart is so massiv that it is nough to mak two nw particls. A quark and an antiquark ar cratd, anothr xampl of pair production. A particl calld a nutral pion is mad from an up quark and an antiup quark. Moving ths apart crats anothr up quark and an antiup quark. W now hav two pairs of quarks. Trying to sparat two quarks mad two mor quarks. Particl Classification Now that w know that quarks ar th smallst building blocks w can sparat all othr particls into two groups, thos mad from quarks and thos that arn t mad from quarks. Hadrons Havy and mad from smallr particls Lptons Light and not mad from smallr particls

4 4 Hadrons To know what a hadron is and th diffrnc btwn th two typs To know th proprtis common to all hadrons To know th structur of th common hadrons and which is th most stabl Mad from Smallr Stuff Hadrons, th Grk for havy ar not fundamntal particls thy ar all mad from smallr particls, quarks. Th proprtis of a hadron ar du to th combind proprtis of th quarks that it is mad from. Thr ar two catgoris of Hadrons: s and Msons. s Mad from thr quarks Proton Nutron u +⅔ +⅓ 0 d -⅓ +⅓ 0 u +⅔ +⅓ 0 u +⅔ +⅓ 0 d -⅓ +⅓ 0 d -⅓ +⅓ 0 p n Th proton is th only stabl hadron, all othrs vntually dcay into a proton. Msons Mad from a quark and an antiquark Pion Plus Pion Minus u +⅔ +⅓ 0 u -⅔ -⅓ 0 d +⅓ -⅓ 0 d -⅓ +⅓ 0 π π Pion Zro Pion Zro u +⅔ +⅓ 0 d -⅓ +⅓ 0 u -⅔ -⅓ 0 d +⅓ -⅓ 0 π π Kaon Plus Kaon Minus u +⅔ +⅓ 0 u -⅔ -⅓ 0 s +⅓ -⅓ +1 s -⅓ +⅓ -1 K K Kaon Zro AntiKaon Zro d -⅓ +⅓ 0 d +⅓ -⅓ 0 s +⅓ -⅓ +1 s -⅓ +⅓ -1 K K Anti Hadrons Anti hadrons ar mad from th opposit quarks as thir Hadron countrparts, for xampl a proton is mad from th quark combination uud and an antiproton is mad from th combination u u d W can s that a π + and a π - ar particl and antiparticl of ach othr. Anti Proton Anti Nutron u -⅔ -⅓ 0 d +⅓ -⅓ 0 u -⅔ -⅓ 0 u -⅔ -⅓ 0 d +⅓ -⅓ 0 d +⅓ -⅓ 0 p n You nd to know all th quark combination shown on this pag as thy may ask you to rcit any of thm!!!!

5 5 Lptons To b abl to xplain what a lpton is To know th proprtis common to all lptons To b abl to xplain th consrvation laws and b abl to us thm Fundamntal Particls A fundamntal particl is a particl which is not mad of anything smallr. s and Msons ar mad from quarks so thy ar not fundamntal, but quarks thmslvs ar. Th only othr known fundamntal particls ar Bosons (s 6: Forcs and Exchang Particls) and Lptons. Lptons Lptons ar a family of particls that ar much lightr than s and Msons and ar not subjct to th strong intraction. Thr ar six lptons in total, thr of thm ar chargd and thr ar unchargd. Th chargd particls ar lctrons, muons and tauons. Th muon and tauon ar similar to th lctron but biggr. Th muon is roughly 200 tims biggr and th tauon is 3500 tims biggr (twic th siz of a proton). Each of th chargd lptons has its own nutrino. If a dcay involvs a nutrino and a muon, it will b a muon nutrino, not a tauon nutrino or lctron nutrino. Th nutrino is a charglss, almost masslss particl. It isn t affctd by th strong intraction or EM forc and barly by gravity. It is almost impossibl to dtct. Lpton Lpton Numbr (L) Anti Lpton Lpton Numbr (L) Elctron Anti Elctron Elctron Nutrino ν 0 +1 Anti Elctron Nutrino ν ē 0-1 Muon μ Anti Muon μ Muon Nutrino ν μ 0 +1 Anti Muon Nutrino ν μ 0-1 Tauon τ Anti Tauon τ Tauon Nutrino ν τ 0 +1 Anti Tauon Nutrino ν τ 0-1 Consrvation Laws For a particl intraction to occur th following laws must b obyd, if ithr is violatd th raction will nvr b obsrvd (will nvr happn): : Must b consrvd (sam total valu bfor as th total valu aftr) Numbr: Must b consrvd Lpton Numbr: Must b consrvd : Consrvd in EM and Strong Intraction. Dosn t hav to b consrvd in Wak Intraction Exampls In pair production a photon of nrgy is convrtd into a particl and its antiparticl γ Q Consrvd B Consrvd L Consrvd S Consrvd Lt us look at bta plus dcay as w knw it at GCSE. A nutron dcays into a proton and rlass an lctron. n p + - Q Consrvd B Consrvd L Not Consrvd S Consrvd This contributd to th sarch for and discovry of th nutrino. Numbr Rmindrs Thr may b a clu to th charg of a particl; π +, K + and + hav a positiv charg. It will only hav a baryon numbr if it IS a baryon. Msons and Lptons hav a Numbr of zro. It will only hav a lpton numbr if it IS a lpton. s and Msons hav a Lpton Numbr of zro. It will only hav a strangnss if it is mad from a strang quark. Lptons hav a strangnss of zro.

6 6 Forcs and Exchang Particls To know th four fundamntal forcs, thir rangs and rlativ strngths To know what ach forc dos and what it acts on To b abl to xplain what xchang particls ar Th Four Intractions Thr ar four forcs in th univrs, som you will hav com across alrady and som will b nw: Th lctromagntic intraction causs an attractiv or rpulsiv forc btwn chargs. Th gravitational intraction causs an attractiv forc btwn masss. Th strong nuclar intraction causs an attractiv (or rpulsiv) forc btwn quarks (and so hadrons). Th wak nuclar intraction dos not caus a physical forc, it maks particls dcay. Wak mans thr is a low probability that it will happn. Intraction/Forc Rang Rlativ Strngth Strong Nuclar ~10-15 m 1 (1) Elctromagntic ~10 2 (0.01) Wak Nuclar ~10-18 m ~10 7 ( ) Gravitational ~10 36 ( ) Exchang Particls In 1935 Japans physicist Hidki Yukawa put forward th ida that th intractions/forcs btwn two particls wr causd by virtual particls bing xchangd btwn th two particls. H was working on th strong nuclar forc which kps protons and nutrons togthr and thorisd that thy wr xchanging a particl back and forth that carrid th forc and kpt thm togthr. This is tru of all th fundamntal intractions. Th gnral trm for xchang particls is bosons and thy ar fundamntal particls lik quarks and lptons. Ic Skating Analogy Imagin two popl on ic skats that will rprsnt th two bodis xprincing a forc. If A throws a bowling ball to B, A slids back whn thy rlas it and B movs back whn thy catch it. Rpatdly throwing th ball back and forth movs A and B away from ach othr, th forc causs rpulsion. Th analogy falls a littl short whn thinking of attraction, but bar with it. Now imagin that A and B ar xchanging a boomrang (bar with it), throwing it bhind thm pushs A towards B, B catchs it from bhind and movs towards A. Th forc causs attraction. Which Particl for What Forc Each of th intractions/forcs has its own xchang particls. Intraction/Forc Exchang Particl What is acts upon Strong Nuclar Gluons btwn quarks Pions btwn s Nuclons (Hadrons) Elctromagntic Virtual Photon d particls Wak Nuclar W + W Z 0 All particls Gravitational Graviton Particls with masss Borrowing Enrgy to Mak Particls Th xchang particls ar mad from borrowd nrgy, borrowd from whr? From nowhr! Yukawa usd th Hisnbrg Uncrtainty Principl to stablish that a particl of mass-nrgy ΔE could xist for a tim Δt as long as E. t h whr h is Planck s constant. This mans that a havy particl can only xist for a short tim whil a lightr particl may xist for longr. h is Planck s Constant, h = 6.63 x J s. In 1947 th xchang particl of th strong nuclar intraction wr obsrvd in a cloud chambr. Lnding Mony Analogy Think of making xchang particls in trms of lnding sombody som mony. If you lnd sombody 50 you would want it paid back fairly soon. If you lnd sombody 50p you would lt thm hav it for longr bfor paying you back.

7 7 Th Strong Intraction To know why a nuclus dosn t tar itslf apart To know why a nuclus dosn t collaps in on itslf To know why th nutron xists in th nuclus Th Strong Intraction Th strong nuclar forc acts btwn quarks. Sinc Hadrons ar th only particls mad of quarks only thy xprinc th strong nuclar forc. In both s and Msons th quarks ar attractd to ach othr by xchanging virtual particls calld gluons. On a largr scal th strong nuclar forc acts btwn th Hadrons thmslvs, kping thm togthr. A pi-mson or pion (π) is xchangd btwn th hadrons. This is calld th rsidual strong nuclar forc. Forc Graphs Nutron-Nutron or Nutron-Proton Hr is th graph of how th forc varis btwn two nutrons or a proton and a nutron as th distanc btwn thm is incrasd. W can s that th forc is vry strongly rpulsiv at sparations of lss than 0.7 fm ( x m). This prvnts all th nuclons from crushing into ach othr. Abov this sparation th forc is strongly attractiv with a pak around 1.3 fm. Whn th nuclons ar sparatd by mor than 5 fm thy no longr xprinc th SNF. Proton-Proton Th forc-sparation graphs for two protons is diffrnt. Thy both attract ach othr du to th SNF but thy also rpl ach othr du to th lctromagntic forc which causs two lik chargs to rpl. Graph A Graph B Graph C Graph A shows how th strong nuclar forc varis with th sparation of th protons Graph B shows how th lctromagntic forc varis with th sparation of th protons Graph C shows th rsultant of ths two forcs: rpulsiv at sparations lss than 0.7 fm, attractiv up to 2 fm whn th forc bcoms rpulsiv again. Nutrons Nuclar Cmnt In th lightr lmnts th numbr of protons and nutrons in th nuclus is th sam. As th nuclus gts biggr mor nutrons ar ndd to kp it togthr. Adding anothr proton mans that all th othr nuclons fl th SNF attraction. It also mans that all th othr protons fl th EM rpulsion. Adding anothr nutron adds to th SNF attraction btwn th nuclons but, sinc it is unchargd, it dos not contribut to th EM rpulsion.

8 8 Th Wak Intraction To b abl to writ th quation for alpha and bta dcay To know what a nutrino is and why is must xist To b abl to stat th changs in quarks during bta plus and bta minus dcay Alpha Dcay Whn a nuclus dcays in this way an alpha particl (a hlium nuclus) is jctd from th nuclus. A X 4 4 A Y A Z Z2 2 or X A 4 4 Z Z 2Y2H All th mittd alpha particls travlld at th sam spd, maning thy had th sam amount of nrgy. Th law of consrvation of mass-nrgy is mt, th nrgy of th nuclus bfor th dcay is th sam as th nrgy of th nuclus and alpha particl aftr th dcay. Alpha dcay is NOT du to th wak intraction but Bta dcay IS Bta Dcay and th Nutrino In bta dcay a nutron in th nuclus changs to a proton and rlass a bta particl (an lctron). Th problm with bta dcay was that th lctrons had a rang of nrgis so th law of consrvation of massnrgy is violatd, nrgy disappars. Thr must b anothr particl bing mad with zro mass but variabl spds, th nutrino. W can also s from th particl consrvation laws that this is a forbiddn intraction: n p Q: is consrvd Numbr B: numbr is consrvd Lpton Numbr L: Lpton numbr is NOT consrvd Bta Minus (β ) Dcay In nutron rich nucli a nutron may dcay into a proton, lctron and an anti lctron nutrino. n p Q: is consrvd Numbr B: numbr is consrvd Lpton Numbr L: Lpton numbr is consrvd In trms of quarks bta minus dcay looks lik this: dud uud d u which simplifis to: Q: ⅓ +⅔ 1+0 ⅓ ⅓ is consrvd Numbr B: +⅓ +⅓+0+0 ⅓ ⅓ numbr is consrvd Lpton Numbr L: Lpton numbr is consrvd Bta Plus (β + ) Dcay In proton rich nucli a proton may dcay into a nutron, positron and an lctron nutrino. p n Q: is consrvd Numbr B: numbr is consrvd Lpton Numbr L: Lpton numbr is consrvd In trms of quarks bta plus dcay looks lik this: uud dud u d which simplifis to: Q: +⅔ ⅓+1+0 ⅔ ⅔ is consrvd Numbr B: +⅓ +⅓+0+0 ⅓ ⅓ numbr is consrvd Lpton Numbr L: Lpton numbr is consrvd Th wak intraction is th only intraction that causs a quark to chang into a diffrnt typ of quark. In bta dcay up quarks and down quarks ar changd into on anothr. In som ractions an up or down quark can chang into a strang quark maning strangnss is not consrvd. During th wak intraction thr can b a chang in strangnss of ±1.

9 9 Fynman Diagrams To know what a Fynman diagram shows us To b abl to draw Fynman diagrams to rprsnt intractions and dcays To b abl to stat th corrct xchang particl Fynman Diagrams An Amrican Physicist calld Richard Fynman cam up with a way of visualising forcs and xchang particls. Blow ar som xampls of how Fynman diagrams can rprsnt particl intractions. Th most important things to not whn daling with Fynman diagrams ar th arrows and th xchang particls, th lins do not show us th path that th particls tak only which com in and which go out. Th arrows tll us which particls ar prsnt bfor th intraction and which ar prsnt aftr th intraction. Th wav rprsnts th intraction taking plac with th appropriat xchang particl lablld. Exampls Diagram 1 rprsnts th strong intraction. A proton and nutron ar attractd togthr by th xchang of a nutral pion. Diagram 2 rprsnts th lctromagntic intraction. Two lctrons rpl ach othr by th xchang of a virtual photon. Diagram 3 rprsnts bta minus dcay. A nutron dcays du to th wak intraction into a proton, an lctron and an anti lctron nutrino Diagram 4 rprsnts bta plus dcay. A proton dcays into a nutron, a positron and an lctron nutrino. Diagram 5 rprsnts lctron captur. A proton capturs an lctron and bcoms a nutron and an lctron nutrino. Diagram 6 rprsnts a nutrino-nutron collision. A nutron absorbs a nutrino and forms a proton and an lctron. Diagram 7 rprsnts an antinutrino-proton collision. A proton absorbs an antinutrino and mits a nutron and an lctron. Diagram 8 rprsnts an lctron-proton collision. Thy collid and mit a nutron and an lctron nutrino. Gtting th Exchang Particl Th aspct of Fynman diagrams that studnts oftn struggl with is lablling th xchang particl and th dirction to draw it. Look at what you start with: If it is positiv and bcoms nutral you can think of it as throwing away its positiv charg so th boson will b positiv. This is th cas in lctron captur. If it is positiv and bcoms nutral you can think of it as gaining ngativ to nutralis it so th boson will b ngativ. This is th cas in lctron-proton collisions. If it is nutral and bcoms positiv w can think of it ithr as gaining positiv (W+ boson) or losing ngativ (W boson in th opposit dirction). Work out whr th charg is going and labl it.

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

A=P=E M-A=N Alpha particle Beta Particle. Periodic table Nam Pr. Atomic Structur/Nuclar Chmistry (Ch. 3 & 21) OTHS Acadmic Chmistry Objctivs: Undrstand th xprimntal dsign and conclusions usd in th dvlopmnt of modrn atomic thory, including Dalton's Postulats,

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

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

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

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

The van der Waals interaction 1 D. E. Soper 2 University of Oregon 20 April 2012 Th van dr Waals intraction D. E. Sopr 2 Univrsity of Orgon 20 pril 202 Th van dr Waals intraction is discussd in Chaptr 5 of J. J. Sakurai, Modrn Quantum Mchanics. Hr I tak a look at it in a littl mor

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

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

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

ph People Grade Level: basic Duration: minutes Setting: classroom or field site ph Popl Adaptd from: Whr Ar th Frogs? in Projct WET: Curriculum & Activity Guid. Bozman: Th Watrcours and th Council for Environmntal Education, 1995. ph Grad Lvl: basic Duration: 10 15 minuts Stting:

More information

Precision Standard Model Tests (at JLab)

Precision Standard Model Tests (at JLab) Prcision Standard Modl Tsts (at JLab) Xiaochao Zhng Jun 21st, 2018 Th Standard Modl of Particl Physics How should w sarch for nw physics? Prcision SM tsts at Jffrson Lab Qwak, PVDIS Mollr, 12 GV PVDIS

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

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

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

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

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

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

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

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

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

Properties of Quarks ( ) Isospin. π = 1, 1 Proprtis of Quarks Isospin So far, w hav discussd thr familis of lptons but principally concntratd on on doublt of quarks, th u and d. W will now introduc othr typs of quarks, along with th nw quantum

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

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

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

DO PHYSICS ONLINE FROM QUANTA TO QUARKS HIGH ENERGY PARTICLE PHYSICS

DO PHYSICS ONLINE FROM QUANTA TO QUARKS HIGH ENERGY PARTICLE PHYSICS DO PHYSICS ONLINE FROM QUANTA TO QUARKS HIGH ENERGY PARTICLE PHYSICS THE STANDARD MODEL OF MATTER Th Quanta to Quarks option consists of a numbr of parts, som of which concrn th "Standard Modl" of subatomic

More information

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

Give the letter that represents an atom (6) (b) Atoms of A and D combine to form a compound containing covalent bonds. 1 Th diagram shows th lctronic configurations of six diffrnt atoms. A B C D E F (a) You may us th Priodic Tabl on pag 2 to hlp you answr this qustion. Answr ach part by writing on of th lttrs A, B, C,

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

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

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

Chapter 13: Radioactivity

Chapter 13: Radioactivity Chaptr 13: Radioactivity 13.1 Radioactivity Dcay L.O 13.1.1 Explain and dcays Radioactivity / Radioactiv dcay is disintgration of unstabl nuclus to a mor stabl daughtr nuclid with th mission of alpha,

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

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

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

Brief Introduction to Statistical Mechanics

Brief Introduction to Statistical Mechanics Brif Introduction to Statistical Mchanics. Purpos: Ths nots ar intndd to provid a vry quick introduction to Statistical Mchanics. Th fild is of cours far mor vast than could b containd in ths fw pags.

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

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

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

GEOMETRICAL PHENOMENA IN THE PHYSICS OF SUBATOMIC PARTICLES. Eduard N. Klenov* Rostov-on-Don, Russia

GEOMETRICAL PHENOMENA IN THE PHYSICS OF SUBATOMIC PARTICLES. Eduard N. Klenov* Rostov-on-Don, Russia GEOMETRICAL PHENOMENA IN THE PHYSICS OF SUBATOMIC PARTICLES Eduard N. Klnov* Rostov-on-Don, Russia Th articl considrs phnomnal gomtry figurs bing th carrirs of valu spctra for th pairs of th rmaining additiv

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

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

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

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

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

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

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

u x v x dx u x v x v x u x dx d u x v x u x v x dx u x v x dx Integration by Parts Formula

u x v x dx u x v x v x u x dx d u x v x u x v x dx u x v x dx Integration by Parts Formula 7. Intgration by Parts Each drivativ formula givs ris to a corrsponding intgral formula, as w v sn many tims. Th drivativ product rul yilds a vry usful intgration tchniqu calld intgration by parts. Starting

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

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

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

Gradebook & Midterm & Office Hours

Gradebook & Midterm & Office Hours Your commnts So what do w do whn on of th r's is 0 in th quation GmM(1/r-1/r)? Do w nd to driv all of ths potntial nrgy formulas? I don't undrstand springs This was th first lctur I actually larnd somthing

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

hep-lat/ Dec 93

hep-lat/ Dec 93 GLUON VERSUS MESON EXCHANGE IN HADRON-HADRON SYSTEMS ON THE LATTICE 1 H. MARKUM, K. RABITSCH, W. SAKULER Institut fur Krnphysik, Tchnisch Univrsitat Win A-100 Vinna, Austria hp-lat/931059 15 Dc 93 Th intraction

More information

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

Where k is either given or determined from the data and c is an arbitrary constant. Exponntial growth and dcay applications W wish to solv an quation that has a drivativ. dy ky k > dx This quation says that th rat of chang of th function is proportional to th function. Th solution is

More information

CHAPTER 33: PARTICLE PHYSICS

CHAPTER 33: PARTICLE PHYSICS Collg Physcs Studnt s Manual Chaptr 33 CHAPTER 33: PARTICLE PHYSICS 33. THE FOUR BASIC FORCES 4. (a) Fnd th rato of th strngths of th wak and lctromagntc forcs undr ordnary crcumstancs. (b) What dos that

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

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

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

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

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

Low-energy QED tests (and what we can learn from them) Low-nrgy QED tsts (and what w can larn from thm) (0γ) 2γ (4γ) (1γ) 3γ (5γ) Indirct Sarchs for Nw Physics at th tim of LHC Flornc, March 2010 Andrzj Czarncki U. of Albrta & CERN Outlin Gyromagntic factors

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

Brief Notes on the Fermi-Dirac and Bose-Einstein Distributions, Bose-Einstein Condensates and Degenerate Fermi Gases Last Update: 28 th December 2008

Brief Notes on the Fermi-Dirac and Bose-Einstein Distributions, Bose-Einstein Condensates and Degenerate Fermi Gases Last Update: 28 th December 2008 Brif ots on th Frmi-Dirac and Bos-Einstin Distributions, Bos-Einstin Condnsats and Dgnrat Frmi Gass Last Updat: 8 th Dcmbr 8 (A)Basics of Statistical Thrmodynamics Th Gibbs Factor A systm is assumd to

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

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

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

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

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

Higher order derivatives

Higher order derivatives Robrto s Nots on Diffrntial Calculus Chaptr 4: Basic diffrntiation ruls Sction 7 Highr ordr drivativs What you nd to know alrady: Basic diffrntiation ruls. What you can larn hr: How to rpat th procss of

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

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

Outline. Thanks to Ian Blockland and Randy Sobie for these slides Lifetimes of Decaying Particles Scattering Cross Sections Fermi s Golden Rule

Outline. Thanks to Ian Blockland and Randy Sobie for these slides Lifetimes of Decaying Particles Scattering Cross Sections Fermi s Golden Rule Outlin Thanks to Ian Blockland and andy obi for ths slids Liftims of Dcaying Particls cattring Cross ctions Frmi s Goldn ul Physics 424 Lctur 12 Pag 1 Obsrvabls want to rlat xprimntal masurmnts to thortical

More information

SPH4U Electric Charges and Electric Fields Mr. LoRusso

SPH4U Electric Charges and Electric Fields Mr. LoRusso SPH4U lctric Chargs an lctric Fils Mr. LoRusso lctricity is th flow of lctric charg. Th Grks first obsrv lctrical forcs whn arly scintists rubb ambr with fur. Th notic thy coul attract small bits of straw

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

surface of a dielectric-metal interface. It is commonly used today for discovering the ways in

surface of a dielectric-metal interface. It is commonly used today for discovering the ways in Surfac plasmon rsonanc is snsitiv mchanism for obsrving slight changs nar th surfac of a dilctric-mtal intrfac. It is commonl usd toda for discovring th was in which protins intract with thir nvironmnt,

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

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

Math 34A. Final Review

Math 34A. Final Review Math A Final Rviw 1) Us th graph of y10 to find approimat valus: a) 50 0. b) y (0.65) solution for part a) first writ an quation: 50 0. now tak th logarithm of both sids: log() log(50 0. ) pand th right

More information

First derivative analysis

First derivative analysis Robrto s Nots on Dirntial Calculus Chaptr 8: Graphical analysis Sction First drivativ analysis What you nd to know alrady: How to us drivativs to idntiy th critical valus o a unction and its trm points

More information

What makes laser light special? Lasers. Lasers. Laser history. Lasers are everywhere! Review of atom discharge lamps. So how do we make laser light?

What makes laser light special? Lasers. Lasers. Laser history. Lasers are everywhere! Review of atom discharge lamps. So how do we make laser light? Lasrs Lasrs What is diffrnt/spcial about lasr light. How dos a lasr work. - rviw atomic discharg lamps. - how light intracts with atoms - how ths idas ar usd to mak lasr. "You know, I hav on simpl rqust.

More information

How can I control light? (and rule the world?)

How can I control light? (and rule the world?) How can I control light? (and rul th world?) "You know, I hav on simpl rqust. And that is to hav sharks with frickin' lasr bams attachd to thir hads! - Dr. Evil Phys 230, Day 35 Qustions? Spctra (colors

More information

Molecules and Covalent Bond

Molecules and Covalent Bond Molculs and ovalnt ond Qustion Papr 1 Lvl IGSE Subjct hmistry (0620/0971) Exam oard ambridg Intrnational Examinations (IE) Topic toms, lmnts and compounds Sub-Topic Molculs and covalnt bonds ooklt Qustion

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

Laboratorio di Fisica delle Particelle COSMIC MUONS. Giorgia Albani Daniele Cortinovis Alessandra Gaeta Davide Rozza

Laboratorio di Fisica delle Particelle COSMIC MUONS. Giorgia Albani Daniele Cortinovis Alessandra Gaeta Davide Rozza Laboratorio di Fisica dll Particll COSMIC MUONS Giorgia Albani Danil Cortinovis Alssandra Gata David Rozza Rlazion di laboratorio di: Giorgia Albani, Danil Cortinovis, Alssandra Gata, David Rozza ABSTRACT

More information

There is an arbitrary overall complex phase that could be added to A, but since this makes no difference we set it to zero and choose A real.

There is an arbitrary overall complex phase that could be added to A, but since this makes no difference we set it to zero and choose A real. Midtrm #, Physics 37A, Spring 07. Writ your rsponss blow or on xtra pags. Show your work, and tak car to xplain what you ar doing; partial crdit will b givn for incomplt answrs that dmonstrat som concptual

More information

E hf. hf c. 2 2 h 2 2 m v f ' f 2f ' f cos c

E hf. hf c. 2 2 h 2 2 m v f ' f 2f ' f cos c EXPERIMENT 9: COMPTON EFFECT Rlatd Topics Intractions of photons with lctrons, consrvation of momntum and nrgy, inlastic and lastic scattring, intraction cross sction, Compton wavlngth. Principl Whn photons

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

(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

The Compton Effect. c 2 E 1. m e 1 E 1 = 2. c (2) + m e. E e. c 2 E (3)

The Compton Effect. c 2 E 1. m e 1 E 1 = 2. c (2) + m e. E e. c 2 E (3) PHY 19 Compton Effct 1 Th Compton Effct Introduction In this xprimnt w will study two aspcts of th intraction of photons with lctrons. Th first of ths is th Compton ffct namd aftr Arthur Holly Compton

More information