Noether Theorem, Noether Charge and All That

Size: px
Start display at page:

Download "Noether Theorem, Noether Charge and All That"

Transcription

1 Noethe Theoem, Noethe Chage and All That Ceated fo PF by Samalkhaiat 10 Tanfomation Let G be a Lie goup whoe action on Minkowki pace-time fomally ealized by coodinate tanfomation ( ) ( 1,3,η) M i Infiniteimally, we may wite thi a x x = g x, g G (11) x = x + δ x, (1) whee δ x = f ( x; ε) ae mooth function of the coodinate andε 1, = 1,,,dim(G), ae the infiniteimal goup paamete We aume that ou dynamical vaiable (the field) ae decibed by (1,3) n continuou function {1,,, n}, ϕ ( x) l ( M, C ) and tanfom by finite-dimenional ( n n matix) epeentation ρ of the goup (1,3) ( ρ( G), M ), (1,3) G on M : ϕ ( x) ϕ ( x) = D ( g) ϕ ( x), (13) D ( g g ) = D ( g ) D ( g ) (14) t 1 1 t Cloe to the identity element of the goup, ie infiniteimally, we can wite D ( g) = δ + ε ( Σ ), (15) whee the n n matice Σ fom a epeentation of the Lie algeba of the goup Uing (15), we can ewite (13) a [ Σ, ] ic γ Σ β = β Σ γ (16) ( x) = ( x) ( x), (17) δ ϕ ϕ ϕ whee ( x) ( Σ ) ( x) (18) δ ϕ ε ϕ 1

2 Fo late ue, let u now deive ome of the impotant popetie of the vaiation ymbol δ Fom (16) and (18), we ee that γ [ δ, δβ ] ϕ( x) icβ δγ ϕ( x) = (19) Hee, we defined the vaiation ymbol δ by ε δ ( ) = δ ( ) Uing it definition (17), we can eaily how that δ act a deivation on function δ ( f ( x) g( x)) = ( δ f ( x)) g( x) + f ( x)( δ g( x)) (110) Since δ ϕ i witten entiely in tem of the pimay field without time deivative, it (anti)commute with ϕ ( y) at equal time [ δ ϕ( t, x), ϕ ( t, y)] = 0 (111) To fit ode in δ x we can wite ϕ ( x) = ϕ ( x) + δ x ϕ ( x) (11) Uing thi expanion, we can ewite (17) a ( x) = ( x) + x ( x), (113) δ ϕ δϕ δ ϕ whee δϕ ( x) ϕ ( x) ϕ ( x), (114) i the infiniteimal change in the functional fom of field If the field index i a pace-time index taking value in the et {,, ν, νρ,}, in 4- dimenional pace-time δϕ ( x) i nothing but the Lie deivative of a pacetime teno ϕ ( x) with epect to the infiniteimal tanfomation (1) The tanfomation conideed i called pace-time (ymmety) tanfomation if δ x 0 and intenal (ymmety) tanfomation if x δ = 0 ; ( δ δ) i called the obital pat of the (ymmety) tanfomation Commuting both ide of (113) with ϕ ( t, y) (at equal time) and uing (111), we find 0 [ δϕ( t, x), ϕ( t, y)] = δ x [ ϕ( t, x), ϕ( t, y)] ɺ (115)

3 And finally, we note that it will be ueful to wite (113) a an opeato equation with δ = δ + δ x, (116) ( δ, δ ) ae given by thei uual definition on function (17) and (114) Notice that, while δ commute with deivative, δ doe not commute with : [, ] ( x δ δ ) = (117) Execie (11) In D-dimenional Minkowki pace-time, how that ( ) δ x = + ε x + ω x ν + c x ν x η ν x, i the mot geneal olution to the confomal Killing equation ν ν ν ( δ x ) + ( δ x ) = η ( δ x ) D Solution i given in [1] Execie (1) Let f ( x) be a olution to the confomal Killing equation ν f + f = ω( x) g ν ν ν Show that f x ɺ i a contant along the geodeic d dτ Solution: ( ) ( ) ( ) ν 1 f xɺ = xɺ f xɺ = f + f xɺ xɺ = ωg xɺ xɺ = 0 3

4 0 Invaiance of the Action and Noethe Theoem Emmy Noethe [ ] The action [ S :( ρ( G), Ω) R] i given by the integal S ϕ d xl ϕ x ϕ x 4 [ ] = ( ( ), ( )) Ω 4 (1,3) whee Ω R i an abitay, contactible and bounded egion in ( M, η) The Lagangian denity L ( x) i a local eal function of fundamental (pimay) field ϕ ( x), that i, it i contucted fom ϕ ( x) and thei deivative, ϕ, at the ame pace-time point x In ode fo the canonical fomalim to make ene, L ( x) i aumed to contain no econd o highe n 4n deivative of ϕ ( x) and to be at mot quadatic in ϕ ( L : C C R ) It i alo aumed that the field ae well-behaved and vanih ufficiently apidly at infinity Unde the tanfomation (11), a egion (1,3) D M i mapped into a new egion D by point-to-point coepondence Theefoe, infiniteimally g( ε ) induce an infiniteimal change in the egion of integation g( ε): Ω Ω = Ω+ δω 4

5 and map the action integal into g S S = d xl x (1) 4 ( ε): [ ϕ] [ ϕ] ( ) Ω+ δ Ω whee L( x) L ( ϕ ( x), ϕ ( x)) If the action integal i invaiant (ie, S[ ϕ ] = S[ ϕ ], ε andϕ ) unde cetain goup of tanfomation (with paamete ε ), the theoy i aid to have a ymmety coeponding to thoe tanfomation Theefoe, in ode fo the goup G to be a ymmety goup of ou theoy, we mut have δ ( ) d xl( x) = d xl( x) d xl ( x) = 0 () Ω Ω+ δ Ω Ω Changing the dummy integation vaiable in the econd integal, we get 4 4 d x x d x x Ω+ δ Ω Ω L( ) L ( ) = 0 (3) Uing the elation L( x) = L( x) +δl ( x), (4) we can ewite (3) in the fom ( δ ) d x x d x x d xδ x Ω+ Ω Ω Ω We know fom elementay calculu that L( ) L( ) + L ( ) = 0 (5) d dx f ( x) dx f ( x) f ( b) δb f ( a) δa = dx f ( x) δ x dx b+ δb b b a+ δ a a a ( ) (6) Genealizing thi to the 4-dimenional cae in (5), we find (to fit ode in δ x ) that 4 d x( ( Lδ x ) + δl ( x) ) = 0 (7) Ω The ame eult can be obtained if we apply the deivation popety of δ on the left-hand ide of () Uing the elation ( ) ( ) δ d xl( x) = δ d x L( x) + d xδl ( x) = 0 (8) Ω Ω Ω 5

6 det 1 + = exp( T In 1 + ) = exp( T ) 1+ T( ), we can expand the Jacobian of the tanfomation to fit ode a Thu x ρ ρ ρ τ det = det( δ + δ x ) 1+ T( δ x ) = 1+ τδ x x x = det = + ( δ ), δ ( ) = ( δ ) (9) x d x d x d x x d x d x d x x And applying the opeato equation (116) to the Lagangian, give u δ = δ + δ x L L L (10) Putting (9) and (10) in equation (8) give u back equation (7) 4 Since Ω R i an abitay contactible egion, the integand in equation (7) mut vanihe identically ( δ x ) 0 δl+ L (11) Thi i an identity with epect to all it agument, if the goup G i an invaiance goup of the action integal It hold fo all function ϕ ( x), it doe not matte whethe ϕ ( x) ae olution of the Eule-Lagange equation o not Since the divegence tem i not dicaded, the behaviou of ϕ ( x) on the bounday, Ω, i alo ielevant Since [ δ, ] = 0, we can wite L L δl ( x ) = δϕ + ( δϕ ) (1) ϕ ϕ Intoducing the Eule deivative ( ) ˆ δl L L δ S[ ϕ] ˆ =, (13) δϕ ϕ ϕ δϕ into equation (1) and ineting the eulting equation back into equation (11), we aive at the Noethe Identity ˆ δl L δϕ + x L δ + δϕ 0 (14) ˆ δϕ ( ϕ ) Let u aume the field ϕ ( x) ae olution of the Eule-Lagange equation 6

7 ˆ δl = 0, = 1,,, n (15) ˆ δϕ ( x) Thu, the Noethe identity implie that the object (Noethe cuent) L J ( x; ε) L δ x + δϕ, (16) ( ϕ ) atifie the conevation law = 0 (17) J The exitence of the coneved (ymmety) cuent J ( x) i known a the fit Noethe theoem Of coue, phyical cuent do not depend on the paamete of the ymmety goup Indeed, they can be factoed out of equation (16) leaving a goup index on the phyical cuent ( ) L J, 1,,,dim(G) ( ) x = δϕ + L δ x = (18) ( ϕ ) Thu, thee ae a many coneved cuent a thee ae paamete Notice that the coneved cuent i not unique In fact, adding a total divegence of antiymmetic teno to the Noethe cuent doe not poil the conevation law, J = J + F, F = F (19) ν ν ν ( ) ( ) ν ( ) ( ) ( ) ν Quantitie like thee F ae called upe-potential They play impotant ole in the contuction of the coneved chage in geneal elativity and othe geneally covaiant theoie Below, we will ue thi feedom to contuct the ymmetic enegy-momentum teno out of the non-ymmetic canonical teno It will be intuctive to give anothe deivation of the Noethe cuent which i ideologically diffeent fom the one we have jut done It conit in compaing the change δl without uing the equation of motion (ie the off-hell vaiation) with that when the Eule-Lagange equation ae atified (ie with the on-hell vaiation of L ) In thi method, the explicit fom of L a well a δϕ ae aumed known Accoding to (1), an abitay infiniteimal change in the field induce the following change in the Lagangian L L L δl = δϕ + δϕ ϕ ( ϕ) ( ϕ) Uing the equation of motion (ie on-hell), we find 7

8 L δl = δϕ (0) ( ϕ) Thi i alway tue, whethe o not δϕ i a ymmety tanfomation On the othe hand, if without the ue of equation of motion (ie jut by ubtituting δϕ in (1)) the Lagangian change by a total divegence of ome object Λ, L, (1) δ = Λ then the action emain unchanged, and the tanfomation, δϕ, i a ymmety tanfomation of the theoy Fom (19) and (0), it follow that the coneved Noethe cuent i L J ( x) = δϕ Λ ( x) ( ϕ ) () Notice that uing thi method to deive the cuent, you do not need to know how x tanfom unde the ymmety goup in quetion So, how can you ditinguih between intenal and pace-time ymmetie, if you don t have δ x? To anwe thi quetion we ue the fact that adding total divegence to a Lagangian doe not affect the dynamic Indeed, it i alway poible to find a dynamically equivalent Lagangian L ˆ( x) uch that ˆ( x) ( x ) L = L + (3) Thu ˆ δl = δl + δ = ( Λ + δ ) (4) So, if Λ = 0, o it i poible to emove it by a uitable choice of you ae dealing with an intenal ymmety Othewie, it i pace-time ymmety, then 1 Tanlation Invaiance and the Ste Enegy-Momentum Teno Uing the elation δ ϕ = δ ϕ δ ϕ, (5) ν ( x) ( x) x ν ( x) which follow fom (116) when we facto out the infiniteimal paamete ε, we can ewite (18) in the fom 8

9 whee ( ) L J ( ) ( ) x x x ν = δϕ θ ν δ, (6) ( ϕ ) L θ ν ( x) νϕ δ νl ( x) (7) ( ϕ ) Intoducing the canonical conjugate field L( x) π ( x) ɺ ϕ ( x), (8) 00 into the θ component, we find H ɺ L (9) 00 ( x) θ ( x) = π ( x) ϕ( x) ( x) In the claical mechanic of continuou ytem, H ( x) i nothing but the Hamiltonian denity of the ytem Theefoe, it follow fom conideation of ν covaiance that θ epeent the canonical te enegy-momentum teno of the field Let u calculate it divegence on hell, ie by uing the Eule- Lagange equation of motion, ν L ν L ν ν ν L θ = ϕ + ϕ L ( ϕ, ϕ, x) = η ϕ ( ϕ ) x Clealy, thi vanihe (on hell) if the Lagangian doe not depend explicitly on x Thu, the enegy-momentum teno i the coneved Noethe cuent aociated with the ymmety goup of pace-time tanlation Indeed, unde pace-time tanlation ν ν ν ν δ x = ε, δ x = δ (30) And all field, egadle of thei tenoial chaacte, ae invaiant, δ ϕ ( x) = 0 (31) Putting (4) and (5) into the defining equation (0) of J ( )( x), we find J ( x) θ ( x) Thu, it follow tivially fom (17) that the enegy-momentum teno i coneved ν θ ( x) = 0 (3) 9

10 Loentz Invaiance and the field Moment Teno Unde infiniteimal Loentz tanfomation δ x = η ω x, (33) ν ν ρ ρ the field tanfom accoding to i ν δ ϕ( x) = ω ( Σ ν ) ϕ( x), (34) whee Σ ν ae the appopiate (pin) tanfomation matice fo the field ϕ Uing thee elation, we can wite the coneved cuent, (6), in the fom 1 L J = ω ν i ( Σ ) ( x ρ x ρ ν ϕ ηρ θ ν ηνρ θ ) ( ϕ) Thi implie that the moment teno M L = ( η x θ η x θ ) i ( Σ ) ϕ ( ϕ ) ρ ρ ν νρ ρ ν ν = M ν (35) i coneved Thu, a field theoy i Poincae invaiant if and only if The object ν ν ν ν M = θ θ + S = 0 (36) ρν L ν S ( x) i ( Σ ) ϕ( x), (37) ( ϕ ) ρ depend entiely on the intinic popetie (tenoial natue) of the field In claical field theoy, it chaacteize the polaization popetie of the field Thu, it coepond to the pin (angula momentum) of paticle decibed by the quantized field Fo a ingle component field (cala), the (pin) matix Σ vanihe and (35) become M ν = x ν θ x θ ν Thi elation i vey muck like the elation between momentum and obital angula momentum in the claical mechanic of paticle xi p j x j pi = ijk Lk Theefoe, the fit tem in (35), L ν = x ν θ x θ ν, (38) hould coepond to ome intinic obital angula momentum of the field Thu the moment teno 10

11 νρ νρ νρ M = L +S (39) mut be elated the total angula momentum teno of the field Fom (35) and (36) we can clealy ee the connection between the ymmety popetie of the canonical enegy-momentum teno θ ν and the tuctue of the total moment teno M Fo a cala field, ince S 0, νρ νρ = we find that θν = θν On the othe hand, fo abitay multi-component field, θ ν i not neceaily ymmetic Howeve, the Poincae invaiance condition, (36), togethe with the feedom of adding upe-potential to the cuent, (19), allow u to contuct a ymmetic enegy-momentum teno ν ν Since S = S, let u eek fo a quantity F ν uch that ν ν ν S = F F (40) Putting thi in the Poincae invaiance condition (36), we find θ + F = θ + F ν ν ν ν Theefoe, if we et T ν ν ν θ + F, (41) we ee that T = T (4) ν ν Futhemoe the conevation of the canonical enegy-momentum teno, = 0, implie ν θ T ν ν = F (43) Thu, the conevation of the ymmetic teno T ν demand (upe-potential) ν ν F = F (44) Now, we can ue (40) and (44) to olve fo the upe-potential ν 1 ( ν ν ν F = S S + S ) (45) The coneved teno T ν i called the Belinfante ymmetic enegymomentum teno In tem of thi ymmetic teno, the total moment teno become 11

12 M = ( x T x T ) + ( F F S ) + P, ν ν ν ν ν ν ρν ρ P = F x F ρν ρ ν ρν x The quantity in the middle backet vanihe when (40) and (44) ae ued, and if we dop the upe-potential P, we aive at the Belinfante moment teno M ν = x ν T x T ν (46) Notice that the (intenal) pin pat ha diappeaed fom the total moment teno whoe conevation now follow fom the conevation of the ymmetical enegy-momentum teno The phyical impotance of the ymmetical (Belinfante) enegy momentum teno follow fom the belief that gaviton couple to T ν ν, and not to θ Indeed, if the matte theoy i minimally coupled to gavity and it action i vaied with epect to the metic teno g ν, the ymmetic enegy momentum teno i obtained in the limit g ν η ν δ D T = d x ( ϕ, ϕ, g ) ν ν g δ g L (47) ν With the ymmetical enegy momentum teno, the coneved Poincae cuent take on the compact (Beel-Hagen []) fom Since δ x J T x ν = νδ (48) = + ω x, we can ewite the cuent in the fom ν ν ν λ λ o 1 J ν T ν x T ν T ν = ν + ω ν = ν ω ( xν T x Tν ), (49) J 1 = ν T ω ν ν ν M (50) Taking the divegence of the cuent (48), and uing the ymmety of the enegy momentum teno, we find 1 J ( T ) x ν T ( x ν ν x = ν δ + ν δ + δ ) = 0 The fit tem on the ight hand ide vanihe becaue of T ν = 0, and the econd tem vanihe becaue Poincae tanfomation δ x f ( x) = + ω x ν, (51) ν 1

13 ae the mot geneal olution to the Killing equation (in any numbe of dimenion) Now conide the cuent f + f = 0 (5) ν ν J T x ν = νδ, (53) whee T ν i the coneved and ymmetic enegy momentum teno, and ν ν δ x = f i vecto field atifying the confomal Killing equation in D- dimenional pace-time Taking the divegence of the cuent, we find ν ν ν f + f = f η (54) D f J = T (55) D Thu, the cuent (53) i coneved povided that the coneved and ymmetic enegy momentum teno i tacele T = 0 Indeed, confomal invaiance allow u to futhe impove the Belinfante enegy-momentum teno o that it i tacele much in the ame way that Poincae invaiance allowed u to make the canonical Enegy-momentum teno ymmetic [1] Thi way, the coneved confomal cuent can be witten in the compact Beel-Hagen fom (53) 3 Poincae and Scale Invaiance and the Tacele Enegy Momentum Teno Unde cale (dilatation) tanfomation the field tanfom accoding to x x = e x, δ x = x, (56) and ϕ ϕ = ϕ δ ϕ = ϕ (57) ( ) ( ) d x x e ( x), ( x) d ( x) ( ) δϕ ( x) = d + x ϕ ( x) (58) whee the eal numbe d epeent the caling dimenion of the field ϕ (we aume all component have the ame caling dimenion) In D dimenion, it value fo cala and vecto field, i given by 13

14 D d = (59) Uing (6), we find the canonical dilatation cuent ν L D = θ ν x + dϕ ( ϕ ) (60) Thu L D = θ + dϕ (61) ( ϕ) Theefoe, in cale invaiant theoie, the tace of the canonical enegymomentum teno i given by L θ = dϕ (6) ( ϕ) We will now how that Poincae and cale invaiance allow u to contuct coneved, ymmetic and tacele enegy momentum teno Recall that fo ν ν any ank-3 teno R = R, anti-ymmetic in the lat two indice, the following combination i a teno anti-ymmetic in the fit two indice ν 1 ( ν ν ν ) ν F = R + R R = F (63) Thu, F ν = 0 and the following modified enegy-momentum teno i coneved Taking the tace, T T 1 = θ + ( R + R R ) (64) ν ν ν ν ν = η T, we find ν ν = θ + η R (65) T ν ν Uing the condition fo cale invaiance, (6), the tace become T L = η R dϕ (66) ( ϕ) ν ν Recall that, in ode to ymmetize the enegy-momentum teno, Poincae ν ν invaiance allowed u to chooe R = S, ee (45) So, fo Poincae and 14

15 cale invaiant theoie, tacele enegy-momentum teno can be obtained by witing ν ν 1 ν ν R = S + ( η V η V ), (67) D 1 whee the vecto field V i detemined fom (66) by etting T = 0: L V = dϕ η ( ρϕ) νρ ρ νs (68) Notice that fo a cala field, the pin matix vanihe Thu fom (37) we find S ν = 0 Theefoe, if we conide the cale invaiant field theoy we find D 1 ν D L = ην ϕ ϕ λϕ, (69) D D ϕ ϕ 4 4 V =, V = (70) Thu, the coneved, ymmetic and tacele enegy-momentum teno i D 4( D 1) ( η ) ν ν ν ν T = T + ϕ, (71) whee T ν i the ymmetic enegy-momentum teno T ν = ϕ ν ϕ L (7) Execie (1) Show that the enegy momentum teno (71), i coneved, ν ν T = 0 and tacele, η T = 0 Execie () Conide the fee Maxwell theoy in D-dimenional pace-time ν 1 L = 4 F F ν ν Show that the ymmetic, coneved enegy momentum teno i given by the Belifante expeion in any numbe of dimenion but tacele only in 4 dimenion 1 T F F F 4 ν ν ν = + η, 15

16 T D = 1 F 4 Execie (3) Show that Maxwell theoy i cale invaiant in any numbe of dimenion Given that D δ A = x + A Show that (up to a tivially coneved upe potential) the coneved dilation cuent i given by ν 4 D ν D = T ν x + F Aν By explicit calculation, how that D = 0 4 The New Impoved CCJ teno [3] and the Belinfante teno fom the action: fun with upe-potential Baically, thi ubection i about obtaining the eult of the lat two ubection fom vaying the action integal Recall that on-hell, the vaiation of the action can be witten a L δ = δ ϕ θ δ 4 ν S d x x ν ( ϕ) (73) To thi vaiation, we will add zeo and how that the coefficient of δ x ν i the new impoved enegy-momentum teno of Callan, Coleman and Jackiw [3] Conide the functional ( ), 4 R = d x Γ x whee Γ i a local function of the field and it deivative to finite ode We vay thi uing (110), 4 4 δ R = δ d x Γ+ d xδ Γ ( ) ( ) If in the fit integal we make ue of (9), and in the econd integal we ue (116), we find 16

17 ( )( ) ( ) ( )( ) R = d x x Γ + d x Γ + d x x Γ δ δ δ δ Combining the fit and the thid tem and uing [ δ, ] = 0 in the econd tem, we get ρ ( ρ ) R = d x Γ + x Γ (74) 4 δ δ δ Uing (116) again, thi can be ewitten a ρ ρ τ ( ( ) ) 4 δ R = d x δ Γ + δτ ργ δτ ργ δ x (75) Integating the econd tem by pat, we find ρ ρ τ ρ ρ { ( ) } ( ) δ R = d x δ Γ δ Γ δ Γ δ x + δ x Γ δ x Γ 4 τ τ ρ ρ The econd tem vanihe identically, and we ae left with ρ ρ τ { ( ) } 4 δ R = d x δ Γ δτ Γ δτ Γ ρδ x (76) Now, we add (76) and ubtact (75) fom (73) 4 L ρ ρ τ δ S = d x δ ϕ ( δτ Γ δτ Γ ) ρδ x ( ϕ) ρ ρ τ {( θ δ δ ) δ x } 4 d x τ + τ ργ τ ργ (77) Let u aume that ou ymmety tanfomation change the action accoding to Now, if we can find Γ uch that S d x ( x) (78) 4 δ = Λ L ( ϕ ) ( ) Γ Γ x = Λ (, ) ρ ρ τ δ ϕ δτ δτ ρδ ϕ ϕ, (79) hold, then the Noethe cuent will have the Beel-Hagen fom τ J = T τδ x, (80) with a new impoved enegy-momentum teno given by T ( ) = θ + η Γ η Γ (81) τ τ τ ρ ρτ ρ 17

18 Execie (4) Conide the fee male cala field action in fou dimenion S 1 ϕ ϕ 4 = d x (i) Show that δ S = 0, ie Λ ( x) = 0, unde the Loentz tanfomation δ x = ω δ ϕ = ν ν x, 0 Then how that Loentz invaiance implie the following condition on ν ν Γ = Γ (ii) Show that δ S = 0, Λ = 0, unde the cale tanfomation Γ x = x, = δ δ ϕ ϕ Ue (79) to how that cale invaiance implie 1 6 Γ = ϕ Ue thi to how that (81) lead to the ymmetic and tacele enegymomentum teno T 1 = θ + ( η ) ϕ 6 ν ν ν ν (iii) Show that the confomal tanfomation δ x = x c x c x δ ϕ = c x ϕ, ( ), ( ) change the cala field action by total divegence ( ϕ ) δ S = d x Λ = d x c 4 4 Ue Loentz invaiance and cale invaiance etiction on (79) i atified fo the confomal tanfomation Γ to how that 18

19 30 Canonical Quantization and Equal-Time Commutato Algeba Befoe intoducing the Noethe chage and dicu it popetie, we need to et up ou quantization cheme We will wok with the canonical quantization ule: Poion backet of function goe to equal-time (anti)commutato of the coeponding opeato 1 i{ f ( t, x), g( t, y)} [ fˆ ( t, x), gˆ ( t, y )] PB Howeve, we will not ue the hat to indicate opeato Alo, we will not wite the time agument explicitly Unle tated othewie, all (anti)commutato ae conideed to be at equal time So, fo any local functional F, we ue the following ule δ F( x) i{ F( x), ϕ( y)} PB = i = [ F( x), ϕ( y)], δπ ( y) (31) δ F( x) i{ F( x), π ( y)} PB = i = [ F( x), π ( y)] δϕ ( y) (3) The fundamental equal-time commutation elation follow by putting F = ϕ, π : ϕ π δ δ 3 [ ( x), ( y)] = i ( ), [ ϕ ( x), ϕ ( y)] = [ π ( x), π ( y)] = 0 x y (33) Notice that π ( x) = ( ϕ, ϕ, ɺ ϕ) ɺ ϕ L (34) In mot cae, the Lagangian i quadatic inϕɺ Thu, π i linea inϕɺ We will aume that the imultaneou linea equation (34) can be olved foϕɺ That i we aume that it i poible to epeent the velocity by ome function ɺ ϕ ( x) = f ( ϕ, ϕ, π) (35) The functional deivative of any local function of the field vaiable, uch a the Lagangian, will be calculated uing the chain ule: 1 In ef [4] I have out-lined the poof of lim i ( ˆ ˆ ˆ ˆ ) A AB BA B A = B ħ 0ħ x p p x 19

20 ( x) ( j ϕ) δl( x) L( x) δϕ( x) L( x) δ L( x) δϕɺ ( x) = + +, δϕ ( y) ϕ ( x) δϕ ( y) ( ϕ ) δϕ ( y) ɺ ϕ ( x) δϕ ( y) j L( x) L( x) δϕɺ ( x) = δ ( x y) + δ ( x y) + π ( x), ϕ ( ) ( ϕ ) δϕ ( y) 3 ( x) 3 j x j δl( x) L( x) δϕɺ ( x) δϕɺ ( x) = = π ( x) δπ ( y) ɺ ϕ ( x) δπ ( y) δπ ( y) Thu, uing (31) and (3) in the above two equation, we infe the following equal-time commutation elation [ L ( x), ϕ ( y)] = π ( x)[ ɺ ϕ ( x), ϕ ( y)], (36) π δ x y L δ x y L L π ɺ ϕ π (37) 3 ( x) 3 [ ( x), ( y)] = i ( ) + i j ( ) + ( x)[ ( x), ( y)] ϕ ( jϕ) The lat two tem in (37) can be combined to give L( x) L( x) L (38) 3 [ ( x), π ( y)] = i δ ( x y) + [ ϕ( x), π ( y)] ϕ ( x) ( ϕ) We will now ue thee commutation elation togethe with the fundamental equal-time commutation elation (33) to deive few impotant equation Let tat by deiving the o-called Heienbeg equation [ ih, ϕ ( x)] = ɺ ϕ ( x), [ ih, π ( x)] = ɺ π ( x) (39) The HamiltonianH i obtained by integating the Hamiltonian denity which we defined in (9) = d xh x = d xθ x, (310) H ( ) ( ) wheea the 3-momentum of the field i given by = d xθ x (311) j 3 0 j P ( ) So, let u commute the Hamiltonian denity with ϕ ( y) and π ( y) [ H( x), ϕ ( y)] = [ π ( x), ϕ ( y)] ɺ ϕ ( x) + π ( x)[ ɺ ϕ ( x), ϕ ( y)] [ L( x), ϕ ( y)], [ H( x), π ( y)] = π ( x)[ ɺ ϕ ( x), π ( y)] [ L( x), π ( y)] Ineting (36) and (37) and uing (33), we find 0

21 ih x ϕ y = δ x y ɺ ϕ x, (31) 3 [ ( ), ( )] ( ) ( ) L( x) L( x) H π δ x y δ x y (313) 3 ( x) 3 [ i ( x), ( y)] = ( ) + j ( ) ϕ ( jϕ) Integating ove x, we find (afte integating (313) by pat) [ ih, ϕ ( y)] = ɺ ϕ ( y), L( y) L( y) L ( y) [ ih, π ( y)] = j = 0 = ɺ π ( y), ϕ( y) ( jϕ) ɺ ϕ whee the Eule-Lagange equation and the definition of the conjugate momentum (8) have been ued In QFT thee ae called Heienbeg equation which, accoding to (31) and (3), coepond to the canonical Hamilton equation in claical field theoy δh δh = ɺ ϕ( x), = ɺ π( x) (314) δπ ( x) δϕ ( x) In exactly the ame way, we can etablih the following moe geneal equaltime commutation elation iθ x ϕ y = δ x y ϕ x (315) 0 3 [ ( ), ( )] ( ) ( ), iθ x π y = η L( x) η π x δ x y + η L( x) δ x y (316) 0 0 j [ ( ), ( )] ( ) j ( ) ( ) jϕ ϕ Integating thee ove x and intoducing the Eule deivative (13) in (316), we find whee i t ϕ x i d x θ x ϕ x = ϕ x, (317) 3 0 [ P ( ), ( )] [ ( ), ( )] ( ) ˆ [ ip ( t), π ( x)] [ i d x θ ( x ), π ( x)] π ( x) η δ L = +, (318) ˆ δϕ t = d xθ x, (319) 3 0 P ( ) ( ) i the field enegy-momentum 4-vecto We will talk about the phyical meaning of thee elation, and how thatp i indeed a time-independent 4- vecto, when we intoduce the Noethe chage We will alo ee why the Eule-Lagange equation of motion appea in (318) but not in (317) Notice that (318) how the equivalence between Lagangian and Hamiltonian fomalim 1

22 ˆ δl( x) δp = 0 [ ip, π ( x)] = π ( x) = ˆ δϕ ( x) δϕ ( x) (30) Okay, ince we calculated the ETCR of the 0-th component of tanlation 0 cuent, θ, with the field, let u do ome jutice to the Poincae goup and oν do the ame thing with the 0-th component of Loentz cuent M Fom (35) thi i given by M ν ( x) = x ν θ ( x) x θ ν ( x) iπ ( x)( Σ ν ) ϕ( x) (31) Uing (315) and the fundamental ETCR (33), we find ( ) im x ϕ y = x ϕ x ϕ i Σ ϕ x δ x y (3) 0ν ν ν ν 3 [ ( ), l( )] l l ( ) l ( ) ( ) Integating ove x and changing y x, we get ou final eult i t ϕ x i d x M x ϕ x = x ϕ x ϕ i Σ ϕ ν 3 0ν ν ν ν [ M ( ), ( )] [ ( ), ( )] ( ) (33) In the next ection we will how that the integal t = t + t = d xm x, (34) ν ν ν 3 0ν M ( ) L ( ) S ( ) ( ) i a time-independent Loentz teno It epeent the total angula momentum of the field, with the obital angula momentum L ν and the pin angula momentum S ν ae given by ( θ θ ) ν 3 oν 3 0ν ν 0 L ( t) d xl ( x) = d x x ( x) x ( x), ν 3 0ν 3 ν S ( t) d xs ( x) = i d xπ ( x)( Σ ) ϕ( x) (35) Befoe going any futhe, let u make the following obevation: If we contact (317) with the tanlation paamete a and (33) with the Loentz ν paameteω, we ecove the coect infiniteimal Poincae tanfomation on the field δϕ ( x) = [ ia P ( t), ϕ ( x)] = a ϕ ( x), (36) i ν ν i δϕ( x) = [ ω M ν ( t), ϕ( x)] = ω ν x ϕ ( ω Σν ) ϕ( x) i = δ x ϕ ( ω Σ) ϕ( x) Remakably, the only aumption ued to deive thee elation i (that the field atify) the fundamental ETCR (33) Indeed, neithe dynamical conideation (ie, equation of motion) no ymmety conideation (ie, (37)

23 conevation law) have been ued to obtain (36) and (37) In fact we will now how that the ame eult hold fo abitay goup of tanfomation Setting = 0 in the Noethe cuent (18), we find J( )( x) = π ( x) δ ϕ ( x) δ x L ( x) (38) 0 0 Thu, at x = y 0 0 [ J ( x), ϕ ( y)] = π ( x)[ δ ϕ ( x), ϕ ( y)] + [ π ( x), ϕ ( y)] δ ϕ ( x) δ x [ L ( x), ϕ ( y)] 0 0 ( ) Due to (115) and (36) the fit and the thid tem add up to zeo, and the econd tem, when evaluated fom the ETCR (33), give [ ij ( x), ϕ ( y)] = δ ϕ ( x) δ ( x y ) (39) 0 3 ( ) Hence, a 3-volume integation ove x will geneate the infiniteimal tanfomation on the field δ ϕ ( x) = [ iq ( t), ϕ ( x)], (330) whee Q ( t) (the Noethe chage) i given by the integal Q ( t) = d x J ( x) (331) 3 0 ( ) Again, the impotant fact about (330) i that it ha been deived fo abitay goup of tanfomation and without efeence to a pecific fom of L ( x), ie, without any commitment to ymmety o dynamic Theefoe, even when the tanfomation i not a ymmety opeation and at leat fomally, it eem that (330) and it local veion (39) ae alway valid Thu, any eult that can be deived fom them will neceaily be tue if we ignoe the uual difficultie of local quantum field theoy The o-called Wad-Takahahi identity in QFT i jut an altenative fom of the canonical equal-time elation (330) It can be deived fom the following timeodeed poduct ( ) T J ( x) ϕ ( y) = Θ( x y ) J ( x) ϕ ( y) +Θ( y x ) ϕ ( y) J ( x) (33) ( ) ( ) ( ) Diffeentiating thi with epect to x and uing the elation Θ( x y ) = η δ( x y ), ( x) Θ( y x ) = η δ( x y ), ( x) (333) 3

24 we find ( ) ( ) T J ( x) ϕ ( y) = T J ( x) ϕ ( y) + δ ( x y )[ J ( x), ϕ ( y)] (334) ( ) ( ) ( ) The peence of the delta function allow u to ue (39) in the econd tem on the ight and get 4 ( ) ( ) T J ( x) ϕ ( y) = T J ϕ ( y) iδ ( x y) δ ϕ ( x) (335) ( ) ( ) ( ) Now, on integating (335) ove a pace-time egion Ω containing the point y, we aive at the Wad-Takahahi identity 4 4 ( ( ) ) ( ( ) ) Ω (336) Ω iδ ϕ ( y) = d xt J ( x) ϕ ( y) d x T J ( x) ϕ ( y) Since the vaiation δ doe not upet the time odeing, n ( 1 n ) ( 1 i n ) iδt ϕ ( y ) ϕ ( y ) ϕ ( y ) = i T ϕ ( y ) δ ϕ ( y ) ϕ ( y ), (337) 1 n 1 i n i= 1 we can genealize (336) and obtain, fo all yi Ω, a geneal fom fo the W-T identity 4 4 T ( ϕ ( ) ( ) ( ) 1 1) δ ϕ ( ) T ( ) ( 1 1) T ( ) ( 1 1) i i = ϕ ϕ i y y d x J x y d x J x y i= 1 Ω (338) It i clea that the fit tem on the ight hand ide of (336) and (338) vanihe if the cuent i coneved, ie, when the tanfomation i a ymmety tanfomation Let u now go back to (35) and ue it to build up the equal time commutato ν [ im, π ( x)] Fo the pin angula momentum, we find Ω Uing (33), thi become π π ϕ π ν 3 l ν [ is, ( x)] = d x ( x )( Σ ) l [ ( x ), ( x)] ν [ S, ( )] ν i π x = iπ ( x)( Σ ) (339) To calculate the commutato with the obital angula momentum, we multiply (316) by (ix ) and integate ove x Integation by pat then give 3 0ν ν j 0ν L( y) 0ν L( y) [ i d x x θ ( x), π ( y)] = η j ( y π ( y) ) j y η + y η ( jϕ) ϕ 4

25 (340) Uing the identitie η = η ν ν 0 ν j 0 η δ η = δ η ν 0ν jν 0 j j,, (341) in (338), we find afte ome eaangement 3 0ν ν ν 0ν L [ i d xx θ, π ( y)] = η π + y π η δ0 π + δ j ( jϕ) L y η ɺ π L ( ) ( ) 0ν + j ϕ jϕ In thi equation, we ue the definition of the conjugate momentum to obtain L( y) L( y) π ( y) =, ɺ π ( y) = 0 ( 0ϕ ) ( 0ϕ ), (34) L ˆ δl [ i d x x θ, π ( y)] = η π + y π δ η + y η (343) ˆ δϕ 3 0ν ν ν ν 0 ν 0 ( ϕ) Thu, the equied commutato follow by the following anti-ymmetic combination ( ) δl( x) [ il, ( x)] x x ˆ δϕ ˆ ν [ ν ] [ ν ]0 L x [ ν ]0 π = π δ η + η ( ϕ) (344) Adding (34) to (337), we get ν [ M, ν ( )] ν ( ) ( ) ν i x x x x x i ( x)( ) ν π = π π + π Σ + F (345) The exta tem in the Loentz tanfomation law fo π i given by F ˆ δl ( x F ) L ( x = x η δ η ) ˆ δϕ ( ϕ ) ν ν [ ν ]0 [ ν ]0 (346) Thi exta piece doe not vanih even when the equation of motion ae atified Thi i becaue the et{ π ( x)} doe not fom a covaiant manifold unde the Poincae goup 5

26 Now, let u ue Heienbeg equation (39) to pove the following theoem Theoem 31 If the equal-time commutation elation (33) ae valid at a 0 0 cetain time x = y = t, they ae alo valid at t + ε Poof: The poof will be baed on Heienbeg equation and the following Jacobi identity [ ϕ ( x, t),[ ih, π ( y, t)]] + [ π ( y, t),[ ϕ ( x, t), ih]] + [ ih,[ π ( y, t), ϕ ( x, t)]] = Since at x = y = t, we have 3 [ ϕ(, t), π (, t)] = iδ δ ( ) x y x y Thu the thid tem in the Jacobi identity vanihe becaue the delta ae c- numbe And we ae left with [ ϕ ( x, t),[ ih, π ( y, t)]] + [[ ih, ϕ ( x, t)], π ( y, t)] = 0 (347) Uing Heienbeg equation (39) in (345), we find [ ϕ ( x, t), ɺ π ( y, t)] + [ ɺ ϕ ( x, t), π ( y, t)] = 0 (348) Multiplying thi byε and adding the eult to the fundamental equal-time commutation elation, we find ɺ 3 [ ϕ (, ), (, )] [ (, ), (, )] [ (, ), (, )] x t π y t + ϕ x t επ y t + εϕ x t π y t = iδ δ ( x y) (349) Thu, to fit ode inε we can wite thi a ɺ o 3 ( ϕ t εϕ t ) ( π t επ t ) iδ δ ( x, ) + ɺ ( x, ), ( y, ) + ɺ ( y, ) = ( x y), (350) x y x y (351) 3 [ ϕ(, t + ε), π (, t + ε)] = iδ δ ( ) And, by exactly the ame method, we can etablih the emaining commutation elation [ ϕ ( x, t + ε), ϕ ( y, t + ε)] = [ π ( x, t + ε), π ( y, t + ε)] = 0 (35) 6

27 qed Refeence and Futhe Reading [1] Samalkhaiat Confomal Goup, Algeba and Confomal Invaiance in Field Theoy, Phyicfoumcom, thead numbe [] E Beel-Hagen, Math Ann 84, 58 (191) [3] C G Callan, J, S Coleman and R Jackiw, A New Impoved Enegy Momentum Teno, Ann Phy 59, 4 (1970) [4] Samalkhaiat Phyicfoumcom, thead numbe 7

( ) [ ] [ ] [ ] δf φ = F φ+δφ F. xdx.

( ) [ ] [ ] [ ] δf φ = F φ+δφ F. xdx. 9. LAGRANGIAN OF THE ELECTROMAGNETIC FIELD In the pevious section the Lagangian and Hamiltonian of an ensemble of point paticles was developed. This appoach is based on a qt. This discete fomulation can

More information

Gravity. David Barwacz 7778 Thornapple Bayou SE, Grand Rapids, MI David Barwacz 12/03/2003

Gravity. David Barwacz 7778 Thornapple Bayou SE, Grand Rapids, MI David Barwacz 12/03/2003 avity David Bawacz 7778 Thonapple Bayou, and Rapid, MI 495 David Bawacz /3/3 http://membe.titon.net/daveb Uing the concept dicued in the peceding pape ( http://membe.titon.net/daveb ), I will now deive

More information

On the undulatory theory of positive and negative electrons

On the undulatory theory of positive and negative electrons Su la théoie ondulatoie de électon poitif and negatif J. Phy. et le Rad. 7 (1936) 347-353. On the undulatoy theoy of poitive and negative electon By AL. PROCA Intitut Heni Poincaé Pai Tanlated by D. H.

More information

Inference for A One Way Factorial Experiment. By Ed Stanek and Elaine Puleo

Inference for A One Way Factorial Experiment. By Ed Stanek and Elaine Puleo Infeence fo A One Way Factoial Expeiment By Ed Stanek and Elaine Puleo. Intoduction We develop etimating equation fo Facto Level mean in a completely andomized one way factoial expeiment. Thi development

More information

FI 2201 Electromagnetism

FI 2201 Electromagnetism FI Electomagnetim Aleande A. Ikanda, Ph.D. Phyic of Magnetim and Photonic Reeach Goup ecto Analyi CURILINEAR COORDINAES, DIRAC DELA FUNCION AND HEORY OF ECOR FIELDS Cuvilinea Coodinate Sytem Cateian coodinate:

More information

Chapter 19 Webassign Help Problems

Chapter 19 Webassign Help Problems Chapte 9 Webaign Help Poblem 4 5 6 7 8 9 0 Poblem 4: The pictue fo thi poblem i a bit mileading. They eally jut give you the pictue fo Pat b. So let fix that. Hee i the pictue fo Pat (a): Pat (a) imply

More information

The Poisson bracket and magnetic monopoles

The Poisson bracket and magnetic monopoles FYST420 Advanced electodynamics Olli Aleksante Koskivaaa Final poject ollikoskivaaa@gmail.com The Poisson backet and magnetic monopoles Abstact: In this wok magnetic monopoles ae studied using the Poisson

More information

EM Boundary Value Problems

EM Boundary Value Problems EM Bounday Value Poblems 10/ 9 11/ By Ilekta chistidi & Lee, Seung-Hyun A. Geneal Desciption : Maxwell Equations & Loentz Foce We want to find the equations of motion of chaged paticles. The way to do

More information

Section 25 Describing Rotational Motion

Section 25 Describing Rotational Motion Section 25 Decibing Rotational Motion What do object do and wh do the do it? We have a ve thoough eplanation in tem of kinematic, foce, eneg and momentum. Thi include Newton thee law of motion and two

More information

ASTR 3740 Relativity & Cosmology Spring Answers to Problem Set 4.

ASTR 3740 Relativity & Cosmology Spring Answers to Problem Set 4. ASTR 3740 Relativity & Comology Sping 019. Anwe to Poblem Set 4. 1. Tajectoie of paticle in the Schwazchild geomety The equation of motion fo a maive paticle feely falling in the Schwazchild geomety ae

More information

On the integration of the equations of hydrodynamics

On the integration of the equations of hydrodynamics Uebe die Integation de hydodynamischen Gleichungen J f eine u angew Math 56 (859) -0 On the integation of the equations of hydodynamics (By A Clebsch at Calsuhe) Tanslated by D H Delphenich In a pevious

More information

Determining the Best Linear Unbiased Predictor of PSU Means with the Data. included with the Random Variables. Ed Stanek

Determining the Best Linear Unbiased Predictor of PSU Means with the Data. included with the Random Variables. Ed Stanek Detemining te Bet Linea Unbiaed Pedicto of PSU ean wit te Data included wit te andom Vaiable Ed Stanek Intoduction We develop te equation fo te bet linea unbiaed pedicto of PSU mean in a two tage andom

More information

Theorem 2: Proof: Note 1: Proof: Note 2:

Theorem 2: Proof: Note 1: Proof: Note 2: A New 3-Dimenional Polynomial Intepolation Method: An Algoithmic Appoach Amitava Chattejee* and Rupak Bhattachayya** A new 3-dimenional intepolation method i intoduced in thi pape. Coeponding to the method

More information

Fall 2004/05 Solutions to Assignment 5: The Stationary Phase Method Provided by Mustafa Sabri Kilic. I(x) = e ixt e it5 /5 dt (1) Z J(λ) =

Fall 2004/05 Solutions to Assignment 5: The Stationary Phase Method Provided by Mustafa Sabri Kilic. I(x) = e ixt e it5 /5 dt (1) Z J(λ) = 8.35 Fall 24/5 Solution to Aignment 5: The Stationay Phae Method Povided by Mutafa Sabi Kilic. Find the leading tem fo each of the integal below fo λ >>. (a) R eiλt3 dt (b) R e iλt2 dt (c) R eiλ co t dt

More information

Then the number of elements of S of weight n is exactly the number of compositions of n into k parts.

Then the number of elements of S of weight n is exactly the number of compositions of n into k parts. Geneating Function In a geneal combinatoial poblem, we have a univee S of object, and we want to count the numbe of object with a cetain popety. Fo example, if S i the et of all gaph, we might want to

More information

Classical Mechanics Homework set 7, due Nov 8th: Solutions

Classical Mechanics Homework set 7, due Nov 8th: Solutions Classical Mechanics Homewok set 7, due Nov 8th: Solutions 1. Do deivation 8.. It has been asked what effect does a total deivative as a function of q i, t have on the Hamiltonian. Thus, lets us begin with

More information

3. Perturbation of Kerr BH

3. Perturbation of Kerr BH 3. Petubation of Ke BH hoizon at Δ = 0 ( = ± ) Unfotunately, it i technically fomidable to deal with the metic petubation of Ke BH becaue of coupling between and θ Nevethele, thee exit a fomalim (Newman-Penoe

More information

Appendix A. Appendices. A.1 ɛ ijk and cross products. Vector Operations: δ ij and ɛ ijk

Appendix A. Appendices. A.1 ɛ ijk and cross products. Vector Operations: δ ij and ɛ ijk Appendix A Appendices A1 ɛ and coss poducts A11 Vecto Opeations: δ ij and ɛ These ae some notes on the use of the antisymmetic symbol ɛ fo expessing coss poducts This is an extemely poweful tool fo manipulating

More information

Basic propositional and. The fundamentals of deduction

Basic propositional and. The fundamentals of deduction Baic ooitional and edicate logic The fundamental of deduction 1 Logic and it alication Logic i the tudy of the atten of deduction Logic lay two main ole in comutation: Modeling : logical entence ae the

More information

ON THE TWO-BODY PROBLEM IN QUANTUM MECHANICS

ON THE TWO-BODY PROBLEM IN QUANTUM MECHANICS ON THE TWO-BODY PROBLEM IN QUANTUM MECHANICS L. MICU Hoia Hulubei National Institute fo Physics and Nuclea Engineeing, P.O. Box MG-6, RO-0775 Buchaest-Maguele, Romania, E-mail: lmicu@theoy.nipne.o (Received

More information

Quantum theory of angular momentum

Quantum theory of angular momentum Quantum theoy of angula momentum Igo Mazets igo.mazets+e141@tuwien.ac.at (Atominstitut TU Wien, Stadionallee 2, 1020 Wien Time: Fiday, 13:00 14:30 Place: Feihaus, Sem.R. DA gün 06B (exception date 18 Nov.:

More information

PROBLEM SET #1 SOLUTIONS by Robert A. DiStasio Jr.

PROBLEM SET #1 SOLUTIONS by Robert A. DiStasio Jr. POBLM S # SOLUIONS by obet A. DiStasio J. Q. he Bon-Oppenheime appoximation is the standad way of appoximating the gound state of a molecula system. Wite down the conditions that detemine the tonic and

More information

Physics 161 Fall 2011 Extra Credit 2 Investigating Black Holes - Solutions The Following is Worth 50 Points!!!

Physics 161 Fall 2011 Extra Credit 2 Investigating Black Holes - Solutions The Following is Worth 50 Points!!! Physics 161 Fall 011 Exta Cedit Investigating Black Holes - olutions The Following is Woth 50 Points!!! This exta cedit assignment will investigate vaious popeties of black holes that we didn t have time

More information

A Relativistic Electron in a Coulomb Potential

A Relativistic Electron in a Coulomb Potential A Relativistic Electon in a Coulomb Potential Alfed Whitehead Physics 518, Fall 009 The Poblem Solve the Diac Equation fo an electon in a Coulomb potential. Identify the conseved quantum numbes. Specify

More information

As is natural, our Aerospace Structures will be described in a Euclidean three-dimensional space R 3.

As is natural, our Aerospace Structures will be described in a Euclidean three-dimensional space R 3. Appendix A Vecto Algeba As is natual, ou Aeospace Stuctues will be descibed in a Euclidean thee-dimensional space R 3. A.1 Vectos A vecto is used to epesent quantities that have both magnitude and diection.

More information

Static Electric Fields. Coulomb s Law Ε = 4πε. Gauss s Law. Electric Potential. Electrical Properties of Materials. Dielectrics. Capacitance E.

Static Electric Fields. Coulomb s Law Ε = 4πε. Gauss s Law. Electric Potential. Electrical Properties of Materials. Dielectrics. Capacitance E. Coulomb Law Ε Gau Law Electic Potential E Electical Popetie of Mateial Conducto J σe ielectic Capacitance Rˆ V q 4πε R ρ v 2 Static Electic Field εe E.1 Intoduction Example: Electic field due to a chage

More information

Solutions Practice Test PHYS 211 Exam 2

Solutions Practice Test PHYS 211 Exam 2 Solution Pactice Tet PHYS 11 Exam 1A We can plit thi poblem up into two pat, each one dealing with a epaate axi. Fo both the x- and y- axe, we have two foce (one given, one unknown) and we get the following

More information

Math 124B February 02, 2012

Math 124B February 02, 2012 Math 24B Febuay 02, 202 Vikto Gigoyan 8 Laplace s equation: popeties We have aleady encounteed Laplace s equation in the context of stationay heat conduction and wave phenomena. Recall that in two spatial

More information

Bogoliubov Transformation in Classical Mechanics

Bogoliubov Transformation in Classical Mechanics Bogoliubov Tranformation in Claical Mechanic Canonical Tranformation Suppoe we have a et of complex canonical variable, {a j }, and would like to conider another et of variable, {b }, b b ({a j }). How

More information

On a quantity that is analogous to potential and a theorem that relates to it

On a quantity that is analogous to potential and a theorem that relates to it Su une quantité analogue au potential et su un théoème y elatif C R Acad Sci 7 (87) 34-39 On a quantity that is analogous to potential and a theoem that elates to it By R CLAUSIUS Tanslated by D H Delphenich

More information

Geometry of the homogeneous and isotropic spaces

Geometry of the homogeneous and isotropic spaces Geomety of the homogeneous and isotopic spaces H. Sonoda Septembe 2000; last evised Octobe 2009 Abstact We summaize the aspects of the geomety of the homogeneous and isotopic spaces which ae most elevant

More information

Quantum Mechanics II

Quantum Mechanics II Quantum Mechanics II Pof. Bois Altshule Apil 25, 2 Lectue 25 We have been dicussing the analytic popeties of the S-matix element. Remembe the adial wave function was u kl () = R kl () e ik iπl/2 S l (k)e

More information

Symmetry of Lagrangians of holonomic systems in terms of quasi-coordinates

Symmetry of Lagrangians of holonomic systems in terms of quasi-coordinates Vol 18 No 8, Augut 009 c 009 Chin. Phy. Soc. 1674-1056/009/1808/3145-05 Chinee Phyic B an IOP Publihing Lt Symmety of Lagangian of holonomic ytem in tem of quai-cooinate Wu Hui-Bin an Mei Feng-Xiang School

More information

A New Approach to General Relativity

A New Approach to General Relativity Apeion, Vol. 14, No. 3, July 7 7 A New Appoach to Geneal Relativity Ali Rıza Şahin Gaziosmanpaşa, Istanbul Tukey E-mail: aizasahin@gmail.com Hee we pesent a new point of view fo geneal elativity and/o

More information

On a proper definition of spin current

On a proper definition of spin current On a pope definition of pin cuent Qian Niu Univeity of Texa at Autin P. Zhang, Shi, Xiao, and Niu (cond-mat 0503505) P. Zhang and Niu (cond-mat/0406436) Culce, Sinova, Sintyn, Jungwith, MacDonald, and

More information

Precision Spectrophotometry

Precision Spectrophotometry Peciion Spectophotomety Pupoe The pinciple of peciion pectophotomety ae illutated in thi expeiment by the detemination of chomium (III). ppaatu Spectophotomete (B&L Spec 20 D) Cuvette (minimum 2) Pipet:

More information

Physics 506 Winter 2006 Homework Assignment #9 Solutions

Physics 506 Winter 2006 Homework Assignment #9 Solutions Physics 506 Winte 2006 Homewok Assignment #9 Solutions Textbook poblems: Ch. 12: 12.2, 12.9, 12.13, 12.14 12.2 a) Show fom Hamilton s pinciple that Lagangians that diffe only by a total time deivative

More information

22.615, MHD Theory of Fusion Systems Prof. Freidberg Lecture 18

22.615, MHD Theory of Fusion Systems Prof. Freidberg Lecture 18 .65, MHD Theoy of Fuion Sytem Pof. Feidbeg Lectue 8. Deive δw fo geneal cew pinch. Deive Suydam citeion Scew Pinch Equilibia μ p + + ( ) = μ J = μ J= Stability ( ) m k ξ=ξ e ι +ι ξ=ξ e +ξ e +ξ e =ξ +ξ

More information

Physics 121 Hour Exam #5 Solution

Physics 121 Hour Exam #5 Solution Physics 2 Hou xam # Solution This exam consists of a five poblems on five pages. Point values ae given with each poblem. They add up to 99 points; you will get fee point to make a total of. In any given

More information

On Locally Convex Topological Vector Space Valued Null Function Space c 0 (S,T, Φ, ξ, u) Defined by Semi Norm and Orlicz Function

On Locally Convex Topological Vector Space Valued Null Function Space c 0 (S,T, Φ, ξ, u) Defined by Semi Norm and Orlicz Function Jounal of Intitute of Science and Technology, 204, 9(): 62-68, Intitute of Science and Technology, T.U. On Locally Convex Topological Vecto Space Valued Null Function Space c 0 (S,T, Φ, ξ, u) Defined by

More information

PHYS833 Astrophysics of Compact Objects Notes Part 12

PHYS833 Astrophysics of Compact Objects Notes Part 12 1 PHYS833 Atophyic of Compact Object Note Pat 1 Black Hole If the coe of a maive ta gow too lage to fom a neuton ta then thee i nothing that can top it collaping to vey high denity The gavitational field

More information

Many Electron Atoms. Electrons can be put into approximate orbitals and the properties of the many electron systems can be catalogued

Many Electron Atoms. Electrons can be put into approximate orbitals and the properties of the many electron systems can be catalogued Many Electon Atoms The many body poblem cannot be solved analytically. We content ouselves with developing appoximate methods that can yield quite accuate esults (but usually equie a compute). The electons

More information

4. Electrodynamic fields

4. Electrodynamic fields 4. Electodynamic fields D. Rakhesh Singh Kshetimayum 1 4.1 Intoduction Electodynamics Faaday s law Maxwell s equations Wave equations Lenz s law Integal fom Diffeential fom Phaso fom Bounday conditions

More information

13. Adiabatic Invariants and Action-Angle Variables Michael Fowler

13. Adiabatic Invariants and Action-Angle Variables Michael Fowler 3 Adiabatic Invaiants and Action-Angle Vaiables Michael Fowle Adiabatic Invaiants Imagine a paticle in one dimension oscillating back and foth in some potential he potential doesn t have to be hamonic,

More information

Appendix B The Relativistic Transformation of Forces

Appendix B The Relativistic Transformation of Forces Appendix B The Relativistic Tansfomation of oces B. The ou-foce We intoduced the idea of foces in Chapte 3 whee we saw that the change in the fou-momentum pe unit time is given by the expession d d w x

More information

Question 1: The dipole

Question 1: The dipole Septembe, 08 Conell Univesity, Depatment of Physics PHYS 337, Advance E&M, HW #, due: 9/5/08, :5 AM Question : The dipole Conside a system as discussed in class and shown in Fig.. in Heald & Maion.. Wite

More information

V V The circumflex (^) tells us this is a unit vector

V V The circumflex (^) tells us this is a unit vector Vecto Vecto have Diection and Magnitude Mike ailey mjb@c.oegontate.edu Magnitude: V V V V x y z vecto.pptx Vecto Can lo e Defined a the oitional Diffeence etween Two oint 3 Unit Vecto have a Magnitude

More information

d 2 x 0a d d =0. Relative to an arbitrary (accelerating frame) specified by x a = x a (x 0b ), the latter becomes: d 2 x a d 2 + a dx b dx c

d 2 x 0a d d =0. Relative to an arbitrary (accelerating frame) specified by x a = x a (x 0b ), the latter becomes: d 2 x a d 2 + a dx b dx c Chapte 6 Geneal Relativity 6.1 Towads the Einstein equations Thee ae seveal ways of motivating the Einstein equations. The most natual is pehaps though consideations involving the Equivalence Pinciple.

More information

3D-Central Force Problems I

3D-Central Force Problems I 5.73 Lectue #1 1-1 Roadmap 1. define adial momentum 3D-Cental Foce Poblems I Read: C-TDL, pages 643-660 fo next lectue. All -Body, 3-D poblems can be educed to * a -D angula pat that is exactly and univesally

More information

PHYS 110B - HW #7 Spring 2004, Solutions by David Pace Any referenced equations are from Griffiths Problem statements are paraphrased

PHYS 110B - HW #7 Spring 2004, Solutions by David Pace Any referenced equations are from Griffiths Problem statements are paraphrased PHYS 0B - HW #7 Sping 2004, Solutions by David Pace Any efeenced euations ae fom Giffiths Poblem statements ae paaphased. Poblem 0.3 fom Giffiths A point chage,, moves in a loop of adius a. At time t 0

More information

(read nabla or del) is defined by, k. (9.7.1*)

(read nabla or del) is defined by, k. (9.7.1*) 9.7 Gadient of a scala field. Diectional deivative Some of the vecto fields in applications can be obtained fom scala fields. This is vey advantageous because scala fields can be handled moe easily. The

More information

2. Electrostatics. Dr. Rakhesh Singh Kshetrimayum 8/11/ Electromagnetic Field Theory by R. S. Kshetrimayum

2. Electrostatics. Dr. Rakhesh Singh Kshetrimayum 8/11/ Electromagnetic Field Theory by R. S. Kshetrimayum 2. Electostatics D. Rakhesh Singh Kshetimayum 1 2.1 Intoduction In this chapte, we will study how to find the electostatic fields fo vaious cases? fo symmetic known chage distibution fo un-symmetic known

More information

On the quadratic support of strongly convex functions

On the quadratic support of strongly convex functions Int. J. Nonlinea Anal. Appl. 7 2016 No. 1, 15-20 ISSN: 2008-6822 electonic http://dx.doi.og/10.22075/ijnaa.2015.273 On the quadatic uppot of tongly convex function S. Abbazadeh a,b,, M. Ehaghi Godji a

More information

Problems with Mannheim s conformal gravity program

Problems with Mannheim s conformal gravity program Poblems with Mannheim s confomal gavity pogam Abstact We show that Mannheim s confomal gavity pogam, whose potential has a tem popotional to 1/ and anothe tem popotional to, does not educe to Newtonian

More information

Vector d is a linear vector function of vector d when the following relationships hold:

Vector d is a linear vector function of vector d when the following relationships hold: Appendix 4 Dyadic Analysis DEFINITION ecto d is a linea vecto function of vecto d when the following elationships hold: d x = a xxd x + a xy d y + a xz d z d y = a yxd x + a yy d y + a yz d z d z = a zxd

More information

Histogram Processing

Histogram Processing Hitogam Poceing Lectue 4 (Chapte 3) Hitogam Poceing The hitogam of a digital image with gay level fom to L- i a dicete function h( )=n, whee: i the th gay level n i the numbe of pixel in the image with

More information

Rigid Body Dynamics 2. CSE169: Computer Animation Instructor: Steve Rotenberg UCSD, Winter 2018

Rigid Body Dynamics 2. CSE169: Computer Animation Instructor: Steve Rotenberg UCSD, Winter 2018 Rigid Body Dynamics 2 CSE169: Compute Animation nstucto: Steve Rotenbeg UCSD, Winte 2018 Coss Poduct & Hat Opeato Deivative of a Rotating Vecto Let s say that vecto is otating aound the oigin, maintaining

More information

Review: Electrostatics and Magnetostatics

Review: Electrostatics and Magnetostatics Review: Electostatics and Magnetostatics In the static egime, electomagnetic quantities do not vay as a function of time. We have two main cases: ELECTROSTATICS The electic chages do not change postion

More information

Energy Levels Of Hydrogen Atom Using Ladder Operators. Ava Khamseh Supervisor: Dr. Brian Pendleton The University of Edinburgh August 2011

Energy Levels Of Hydrogen Atom Using Ladder Operators. Ava Khamseh Supervisor: Dr. Brian Pendleton The University of Edinburgh August 2011 Enegy Levels Of Hydogen Atom Using Ladde Opeatos Ava Khamseh Supeviso: D. Bian Pendleton The Univesity of Edinbugh August 11 1 Abstact The aim of this pape is to fist use the Schödinge wavefunction methods

More information

arxiv: v2 [gr-qc] 18 Aug 2014

arxiv: v2 [gr-qc] 18 Aug 2014 Self-Consistent, Self-Coupled Scala Gavity J. Fanklin Depatment of Physics, Reed College, Potland, Oegon 970, USA Abstact A scala theoy of gavity extending Newtonian gavity to include field enegy as its

More information

Image Enhancement: Histogram-based methods

Image Enhancement: Histogram-based methods Image Enhancement: Hitogam-baed method The hitogam of a digital image with gayvalue, i the dicete function,, L n n # ixel with value Total # ixel image The function eeent the faction of the total numbe

More information

Physics 2A Chapter 10 - Moment of Inertia Fall 2018

Physics 2A Chapter 10 - Moment of Inertia Fall 2018 Physics Chapte 0 - oment of netia Fall 08 The moment of inetia of a otating object is a measue of its otational inetia in the same way that the mass of an object is a measue of its inetia fo linea motion.

More information

S7: Classical mechanics problem set 2

S7: Classical mechanics problem set 2 J. Magoian MT 9, boowing fom J. J. Binney s 6 couse S7: Classical mechanics poblem set. Show that if the Hamiltonian is indepdent of a genealized co-odinate q, then the conjugate momentum p is a constant

More information

Partition Functions. Chris Clark July 18, 2006

Partition Functions. Chris Clark July 18, 2006 Patition Functions Chis Clak July 18, 2006 1 Intoduction Patition functions ae useful because it is easy to deive expectation values of paametes of the system fom them. Below is a list of the mao examples.

More information

Physics 505 Homework No. 9 Solutions S9-1

Physics 505 Homework No. 9 Solutions S9-1 Physics 505 Homewok No 9 s S9-1 1 As pomised, hee is the tick fo summing the matix elements fo the Stak effect fo the gound state of the hydogen atom Recall, we need to calculate the coection to the gound

More information

ON INDEPENDENT SETS IN PURELY ATOMIC PROBABILITY SPACES WITH GEOMETRIC DISTRIBUTION. 1. Introduction. 1 r r. r k for every set E A, E \ {0},

ON INDEPENDENT SETS IN PURELY ATOMIC PROBABILITY SPACES WITH GEOMETRIC DISTRIBUTION. 1. Introduction. 1 r r. r k for every set E A, E \ {0}, ON INDEPENDENT SETS IN PURELY ATOMIC PROBABILITY SPACES WITH GEOMETRIC DISTRIBUTION E. J. IONASCU and A. A. STANCU Abstact. We ae inteested in constucting concete independent events in puely atomic pobability

More information

Chapter 5 Linear Equations: Basic Theory and Practice

Chapter 5 Linear Equations: Basic Theory and Practice Chapte 5 inea Equations: Basic Theoy and actice In this chapte and the next, we ae inteested in the linea algebaic equation AX = b, (5-1) whee A is an m n matix, X is an n 1 vecto to be solved fo, and

More information

1.2 Differential cross section

1.2 Differential cross section .2. DIFFERENTIAL CROSS SECTION Febuay 9, 205 Lectue VIII.2 Diffeential coss section We found that the solution to the Schodinge equation has the fom e ik x ψ 2π 3/2 fk, k + e ik x and that fk, k = 2 m

More information

Compactly Supported Radial Basis Functions

Compactly Supported Radial Basis Functions Chapte 4 Compactly Suppoted Radial Basis Functions As we saw ealie, compactly suppoted functions Φ that ae tuly stictly conditionally positive definite of ode m > do not exist The compact suppot automatically

More information

I. CONSTRUCTION OF THE GREEN S FUNCTION

I. CONSTRUCTION OF THE GREEN S FUNCTION I. CONSTRUCTION OF THE GREEN S FUNCTION The Helmohltz equation in 4 dimensions is 4 + k G 4 x, x = δ 4 x x. In this equation, G is the Geen s function and 4 efes to the dimensionality. In the vey end,

More information

15 Solving the Laplace equation by Fourier method

15 Solving the Laplace equation by Fourier method 5 Solving the Laplace equation by Fouie method I aleady intoduced two o thee dimensional heat equation, when I deived it, ecall that it taes the fom u t = α 2 u + F, (5.) whee u: [0, ) D R, D R is the

More information

Estimation and Confidence Intervals: Additional Topics

Estimation and Confidence Intervals: Additional Topics Chapte 8 Etimation and Confidence Inteval: Additional Topic Thi chapte imply follow the method in Chapte 7 fo foming confidence inteval The text i a bit dioganized hee o hopefully we can implify Etimation:

More information

Perturbation to Symmetries and Adiabatic Invariants of Nonholonomic Dynamical System of Relative Motion

Perturbation to Symmetries and Adiabatic Invariants of Nonholonomic Dynamical System of Relative Motion Commun. Theo. Phys. Beijing, China) 43 25) pp. 577 581 c Intenational Academic Publishes Vol. 43, No. 4, Apil 15, 25 Petubation to Symmeties and Adiabatic Invaiants of Nonholonomic Dynamical System of

More information

Single Particle State AB AB

Single Particle State AB AB LECTURE 3 Maxwell Boltzmann, Femi, and Bose Statistics Suppose we have a gas of N identical point paticles in a box of volume V. When we say gas, we mean that the paticles ae not inteacting with one anothe.

More information

Simulation of Spatially Correlated Large-Scale Parameters and Obtaining Model Parameters from Measurements

Simulation of Spatially Correlated Large-Scale Parameters and Obtaining Model Parameters from Measurements Simulation of Spatially Coelated Lage-Scale Paamete and Obtaining Model Paamete fom PER ZETTERBERG Stockholm Septembe 8 TRITA EE 8:49 Simulation of Spatially Coelated Lage-Scale Paamete and Obtaining Model

More information

A thermodynamic degree of freedom solution to the galaxy cluster problem of MOND. Abstract

A thermodynamic degree of freedom solution to the galaxy cluster problem of MOND. Abstract A themodynamic degee of feedom solution to the galaxy cluste poblem of MOND E.P.J. de Haas (Paul) Nijmegen, The Nethelands (Dated: Octobe 23, 2015) Abstact In this pape I discus the degee of feedom paamete

More information

arxiv: v1 [math.cv] 7 Nov 2018

arxiv: v1 [math.cv] 7 Nov 2018 INTERMEDIATE HANKEL OPERATORS ON THE FOCK SPACE OLIVIA CONSTANTIN axiv:181103137v1 [mathcv] 7 Nov 2018 Abtact We contuct a natual equence of middle Hankel opeato on the Fock pace, ie opeato which ae intemediate

More information

= e2. = 2e2. = 3e2. V = Ze2. where Z is the atomic numnber. Thus, we take as the Hamiltonian for a hydrogenic. H = p2 r. (19.4)

= e2. = 2e2. = 3e2. V = Ze2. where Z is the atomic numnber. Thus, we take as the Hamiltonian for a hydrogenic. H = p2 r. (19.4) Chapte 9 Hydogen Atom I What is H int? That depends on the physical system and the accuacy with which it is descibed. A natual stating point is the fom H int = p + V, (9.) µ which descibes a two-paticle

More information

This gives rise to the separable equation dr/r = 2 cot θ dθ which may be integrated to yield r(θ) = R sin 2 θ (3)

This gives rise to the separable equation dr/r = 2 cot θ dθ which may be integrated to yield r(θ) = R sin 2 θ (3) Physics 506 Winte 2008 Homewok Assignment #10 Solutions Textbook poblems: Ch. 12: 12.10, 12.13, 12.16, 12.19 12.10 A chaged paticle finds itself instantaneously in the equatoial plane of the eath s magnetic

More information

A hint of renormalization

A hint of renormalization A hint of enomalization Betand Delamotte a) Laboatoie de Phyique Théoique et Haute Enegie, Univeité Pai VI, Piee et Maie Cuie, Pai VII, Deni Dideot, 2 Place Juieu, 75251 Pai Cedex 05, Fance Received 28

More information

Homework 7 Solutions

Homework 7 Solutions Homewok 7 olutions Phys 4 Octobe 3, 208. Let s talk about a space monkey. As the space monkey is oiginally obiting in a cicula obit and is massive, its tajectoy satisfies m mon 2 G m mon + L 2 2m mon 2

More information

you of a spring. The potential energy for a spring is given by the parabola U( x)

you of a spring. The potential energy for a spring is given by the parabola U( x) Small oscillations The theoy of small oscillations is an extemely impotant topic in mechanics. Conside a system that has a potential enegy diagam as below: U B C A x Thee ae thee points of stable equilibium,

More information

Quantum Mechanics I - Session 5

Quantum Mechanics I - Session 5 Quantum Mechanics I - Session 5 Apil 7, 015 1 Commuting opeatos - an example Remine: You saw in class that Â, ˆB ae commuting opeatos iff they have a complete set of commuting obsevables. In aition you

More information

Emerging from Matrix Models

Emerging from Matrix Models fom Matix Models Talk pesented by Daniel N. Blaschke Faculty of Physics, Mathematical Physics Goup Collaboato: H. Steinacke May 15, 2010 1 / 28 1 2 Cuvatue and Actions fo Matix Models 3 4 Reissne-Nodstöm

More information

APPENDIX. For the 2 lectures of Claude Cohen-Tannoudji on Atom-Atom Interactions in Ultracold Quantum Gases

APPENDIX. For the 2 lectures of Claude Cohen-Tannoudji on Atom-Atom Interactions in Ultracold Quantum Gases APPENDIX Fo the lectues of Claude Cohen-Tannoudji on Atom-Atom Inteactions in Ultacold Quantum Gases Pupose of this Appendix Demonstate the othonomalization elation(ϕ ϕ = δ k k δ δ )k - The wave function

More information

Multivariable Control Systems

Multivariable Control Systems Multivaiable Contol Sytem Ali Kaimpou Aociate ofeo Fedowi Univeity of Mahhad Refeence ae appeaed in the lat lide. Stability of Multivaiable Feedback Contol Sytem Topic to be coveed include: Well - oedne

More information

SIMPLE LOW-ORDER AND INTEGRAL-ACTION CONTROLLER SYNTHESIS FOR MIMO SYSTEMS WITH TIME DELAYS

SIMPLE LOW-ORDER AND INTEGRAL-ACTION CONTROLLER SYNTHESIS FOR MIMO SYSTEMS WITH TIME DELAYS Appl. Comput. Math., V.10, N.2, 2011, pp.242-249 SIMPLE LOW-ORDER AND INTEGRAL-ACTION CONTROLLER SYNTHESIS FOR MIMO SYSTEMS WITH TIME DELAYS A.N. GÜNDEŞ1, A.N. METE 2 Abtact. A imple finite-dimenional

More information

Perturbation theory and stability analysis for string-corrected black holes in arbitrary dimensions

Perturbation theory and stability analysis for string-corrected black holes in arbitrary dimensions CPHT-RR-046-0805 SPHT-T05/50 axiv:hep-th/0608009 v Aug 006 Petubation theoy and stability analysis fo sting-coected black holes in abitay dimensions Filipe Moua Cente de Physique Théoique, École Polytéchnique

More information

On the quantum dynamics of wave fields

On the quantum dynamics of wave fields Zu Quantendynami de Wellenfelde Zeit. Py. 56 (99) -6. On te quantum dynamic of wave field By W. Heienbeg in Leipzig and W. Pauli in Zuic (Received on 9 Mac 99) Tanlated by D. H. Delpenic Intoduction. I.

More information

MATH 417 Homework 3 Instructor: D. Cabrera Due June 30. sin θ v x = v r cos θ v θ r. (b) Then use the Cauchy-Riemann equations in polar coordinates

MATH 417 Homework 3 Instructor: D. Cabrera Due June 30. sin θ v x = v r cos θ v θ r. (b) Then use the Cauchy-Riemann equations in polar coordinates MATH 417 Homewok 3 Instucto: D. Cabea Due June 30 1. Let a function f(z) = u + iv be diffeentiable at z 0. (a) Use the Chain Rule and the fomulas x = cosθ and y = to show that u x = u cosθ u θ, v x = v

More information

Two-Body Problem with Varying Mass in Case. of Isotropic Mass Loss

Two-Body Problem with Varying Mass in Case. of Isotropic Mass Loss Adv Theo Appl Mech Vol no 69-8 Two-Body Poblem with Vaying Ma in Cae of Iotopic Ma o W A Rahoma M K Ahmed and I A El-Tohamy Caio Univeity Faculty of Science Dept of Atonomy Caio 6 Egypt FA Abd El-Salam

More information

AST 121S: The origin and evolution of the Universe. Introduction to Mathematical Handout 1

AST 121S: The origin and evolution of the Universe. Introduction to Mathematical Handout 1 Please ead this fist... AST S: The oigin and evolution of the Univese Intoduction to Mathematical Handout This is an unusually long hand-out and one which uses in places mathematics that you may not be

More information

2 Lecture 2: The Bohr atom (1913) and the Schrödinger equation (1925)

2 Lecture 2: The Bohr atom (1913) and the Schrödinger equation (1925) 1 Lectue 1: The beginnings of quantum physics 1. The Sten-Gelach expeiment. Atomic clocks 3. Planck 1900, blackbody adiation, and E ω 4. Photoelectic effect 5. Electon diffaction though cystals, de Boglie

More information

Mechanics Physics 151

Mechanics Physics 151 Mechanics Physics 151 Lectue 5 Cental Foce Poblem (Chapte 3) What We Did Last Time Intoduced Hamilton s Pinciple Action integal is stationay fo the actual path Deived Lagange s Equations Used calculus

More information

J. N. R E DDY ENERGY PRINCIPLES AND VARIATIONAL METHODS APPLIED MECHANICS

J. N. R E DDY ENERGY PRINCIPLES AND VARIATIONAL METHODS APPLIED MECHANICS J. N. E DDY ENEGY PINCIPLES AND VAIATIONAL METHODS IN APPLIED MECHANICS T H I D E DI T IO N JN eddy - 1 MEEN 618: ENEGY AND VAIATIONAL METHODS A EVIEW OF VECTOS AND TENSOS ead: Chapte 2 CONTENTS Physical

More information

Chapter 3: Theory of Modular Arithmetic 38

Chapter 3: Theory of Modular Arithmetic 38 Chapte 3: Theoy of Modula Aithmetic 38 Section D Chinese Remainde Theoem By the end of this section you will be able to pove the Chinese Remainde Theoem apply this theoem to solve simultaneous linea conguences

More information

Stanford University CS259Q: Quantum Computing Handout 8 Luca Trevisan October 18, 2012

Stanford University CS259Q: Quantum Computing Handout 8 Luca Trevisan October 18, 2012 Stanfod Univesity CS59Q: Quantum Computing Handout 8 Luca Tevisan Octobe 8, 0 Lectue 8 In which we use the quantum Fouie tansfom to solve the peiod-finding poblem. The Peiod Finding Poblem Let f : {0,...,

More information

is the instantaneous position vector of any grid point or fluid

is the instantaneous position vector of any grid point or fluid Absolute inetial, elative inetial and non-inetial coodinates fo a moving but non-defoming contol volume Tao Xing, Pablo Caica, and Fed Sten bjective Deive and coelate the govening equations of motion in

More information

one primary direction in which heat transfers (generally the smallest dimension) simple model good representation for solving engineering problems

one primary direction in which heat transfers (generally the smallest dimension) simple model good representation for solving engineering problems CHAPTER 3: One-Dimenional Steady-State Conduction one pimay diection in which heat tanfe (geneally the mallet dimenion) imple model good epeentation fo olving engineeing poblem 3. Plane Wall 3.. hot fluid

More information

B da = 0. Q E da = ε. E da = E dv

B da = 0. Q E da = ε. E da = E dv lectomagnetic Theo Pof Ruiz, UNC Asheville, doctophs on YouTube Chapte Notes The Maxwell quations in Diffeential Fom 1 The Maxwell quations in Diffeential Fom We will now tansfom the integal fom of the

More information