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MIT 8 251 - Lecture Notes

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� � Lecture 14 8.251 Spring 2007 Lecture 14 - Topics Momentum charges for the string • Lorentz charges for the strings • Angular momentum of the rotating string • Discuss α� and the string length �s• General gauges: Fixing τ and natural units • Reading: Section 8.4-8.6 and 9.1 S = dξ0dξ1 . . . dξpL(φa, ∂αφa) ξα: coordinates, φa(ξ): fields, ∂α = ∂ξ∂ α α: coord. index α = 0, 1, . . . , p a: field index a = 1, . . . , m i: index for various symmetries δφa(ξ) =i hai (φ(ξ)) Leaves L invar. to first order. 1. ∂L δφa + ∂L ∂α(δφa) = 0 ∂φa ∂(∂αφa) 3. Jµ Jα iJiα = ∂L δφa ∂(∂αφa) Similar to mechanics: ∂∂Lq˙δq Claim: Given this transformation leaves L invar. to first order then: → i → 2. ∂αJα = 0 ∀i Conserved Current i Check this yourself using 1. and the E − L equations of motion. Done in book as well. Conserved charge too: Qi = JiO(ξ)dξ1dξ2 . . . dξp Answer independent of time. 1� � � Lecture 14 8.251 Spring 2007 dQ = 0 dξO Nambu-Gotta action: S = dξ0 dξ1 L(∂0xµ, ∂1xµ)�������� dτ dσ µThis means α = 0, 1. φa = x a = 0, . . . , d = spatial dimension ⇒Let’s look for asymmetry. A variation of the field that leaves the field invar. δxµ =µ= constant Constant translations of a worldsheet should by asymmetric. Why would Nambu- Gotta action care if rigidally moved worldsheet through time or space? So: δ(∂0xµ) = ∂0(δxµ) = 0 δ(∂1xµ) = 0 So δxµ =µ indeed asymmetric. Apply (3) µJα ∂L µ = µ ∂(∂αxµ) Jα ∂L= µ ∂(∂αxµ) (J0 ∂L ∂L τ σ µ, Jµ1) = ∂x˙µ , ∂x�µ = (P , Pµ )µ Conservation law: ∂αJα = 0 gives us collection of conservation laws for µ. ∂αJα = 0 = ∂Pµτ + ∂Pµa ∂τ ∂a � σ1Pµ(τ ) = 0 Pµτ (τ, σ)dσ conserved quantity indexed by spacetime index µ. Pµ(τ ): conserved momentum for the string not dependent on τ since conserved. Check Pµ is conserved dPµ = � σ1 ∂Pµτ (τ, σ)dσ dτ 0 ∂τ � σ1 ∂Pµσ = − dσ ∂σ 0 = [−Pµσ]σ0 1 2Lecture 14 8.251 Spring 2007 This yields the free BCs. This is the hardest part of the course. After this, it gets easier. A momentum is in general a variation of a Lagrangian with respect to a velocity eg ∂∂x˙Lµ conserved, has units of momentum. We will see this is indeed the relative momentum of a piece of string. When we had (ρ, J�): Q[ρ] =3L[J�] =Q T L2 Now we have (P] = Pµ L , Pmomentum density, and Pσµτµ): [Pτµ[P ] = Pµ Call PT σµτµσµmomentum current. Okay, we have: dPµ = 0 dτ But would like: dPµ = 0 dt Conserved for Lorentz observer. Is this the case? (Yes). dPµSure, could work in static gauge. τ = t dt = 0 ⇒ But what about an arbitrary τ curve on worldsheet? Look for a generalization formula (clue from divergence theorem) A =flux of vector field 3� � � � � � � � � � � � � � Lecture 14 8.251 Spring 2007 ∂Ax ∂Ay (Axdy − Aydx) = + dxdy R ∂x ∂y dτ] =R ∂Pτ + ∂Pσ dτdσ = 0 [Pµτ dσ − Pµσ ∂τ ∂σ Γ Given an arbitrary curve γ, claim momentum given by: Pµ(γ) = [Pµτ dσ − Pµσdτ] γ γ = α → γ2 → β → −γ1 ( γ2 + α + −γ1 + β ) (�Pµτ �� µσdτ �) = 0 dσ − Pκ κ = κ = 0 α β Pµ(γ1) = Pµ(γ2) � σ1Usually will use Pµ(τ) = 0 Pµτ (τ, σ)dτ with constant τ, but nice to have this general formulation. 4Lecture 14 8.251 Spring 2007 Lorentz Transformation xµ = Lνµx ν Leaves ηµν xµxν invar. Vary xµ subject to xν δxµ =µα xα µx ν ) = 2ηµα νδ(ηµν xµν xαx = 2µαxαxµ where ηµν xν = xµ µIf we want δ(ηµν x xν ) = 0, we make antisymmetric. µν νµ = −Claim: δ(ηµν ∂αxµ∂β x ν ) = 0 So Nambu-Gotta action invar and get new set of symmetries: δxµ(τ, σ) =µν xν (τ, σ) µν Jα ∂L α αµν µν = ∂(∂αxµ) δxµ = Pµ δxµ = Pµ xν 1 µν µν Jα α α µν = − 2(xµPν − xν Pµ ) No physical relevance to − 1 2 So define: m α (τ, σ) = xµPα α µν ν − xν Pµ αConserved currents: ∂αmµν = 0 � σ1 Mµν = mµν 0 dσ 0 Conserved Charge � σ � σ1 Mij = mij dσ = (xiPjτ − xj Piτ )dσ = ijk Lk 0 0 123 = +1, totally antisymmetric. eg: 5Lecture 14 8.251 Spring 2007 � σ1 M12 = (x1P2 τ − x2P1 τ )dσ = 12l Lk = L3 0 L�= �r × p�So Mij =angular momentum, conserved. Angular momentum of rotating string: � σ1 M12 = L3 = J = (x1P2 τ − x2P1 τ )dσ 0 � �� � � � �� �x(t, σ) = σ1 cos πσ cos πct , sin πct π σ1 σ1 σ1 Parametrized String � � � � �� �τ = T0 ∂�x = T0 cos πσ − sin πct , cos πct Pc2 ∂t c σ1 σ1 σ1 � �2 � � σ1 T02 πσ x1P2 − x2P1 = cosπ c σ1 1 J = E2 2πT0c E = σ1T0


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MIT 8 251 - Lecture Notes

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