DOC PREVIEW
MIT 8 821 - Problem Set 5

This preview shows page 1 out of 4 pages.

Save
View full document
View full document
Premium Document
Do you want full access? Go Premium and unlock all 4 pages.
Access to all documents
Download any document
Ad free experience
Premium Document
Do you want full access? Go Premium and unlock all 4 pages.
Access to all documents
Download any document
Ad free experience

Unformatted text preview:

MIT OpenCourseWarehttp://ocw.mit.edu 8.821 String Theory Fall 2008 For information about citing these materials or our Terms of Use, visit: http://ocw.mit.edu/terms.� MASSACHUSETTS INSTITUTE OF TECHNOLOGY Department of Physics String Theory (8.821) – Prof. J. McGreevy – Fall 2008 Problem Set 5 Finally, we can calculate 1. Bulk vector fields. a) Use the inversion trick to show that KAM (w, �x) = cD (w − w�x0 D)−2(1 D−1) JAM (w − �x) (where wA ≡ (w0, �w)A labels a point in the bulk of AdSD+1) is the bulk-to-boundary propagator for a massless vector field, i.e. this object solves the bulk Maxwell equations, and → δD(w� − �x) as w0 → 0. Here M JM (x) ≡ δM xAx.A A − 2 x2 Show that JAM (x) = x�2 ∂xA with x A = x�A ∂xM � x2 so this JAM is the Jacobian for the inversion transformation. b) Check that the gravity calculation of three point function �OΔ(x1)OΔ(x2)J µ(x3)� (J µ is the conserved current to which the bulk gauge field AA couples) has the form required by conformal symmetry given in lecture. c) [extra bonus problem] Show that the form of the three point function above is determined by conformal invariance up to a constant. 2. Relation between AdS propagators. Show that the bulk-to-boundary and boundary-to-boundary propagators for a scalar field in AdS are related by KΔ(z, x; x�) = limΔ+ − Δ− GΔ(z, x; z�, x�). z�→� �Δ 1� � � � � Hint: use ‘Green’s second identity’ √g � φ(� − m 2)ψ − ((� − m 2)φ)ψ) � = √γ (φn ∂ψ − (n ∂φ)ψ) ∀φ, ψ · · U ∂U with φ = G, ψ = K. The G appearing in this relation is defined to be the normalizable solution to the wave-equation-with-source � � 1�x − m 2 G(z, x; z�, x�) = √gδD(x − x�)δ(z − z�) which is regular in the interior; K is defined to be the solution to the homoge-neous wave equation which is regular in the interior and approaches lim KΔ(z, x; x�) = �Δ− δD x − x�. z �→[Note: it is possible to show this using properties of the hypergeometric function appearing in the explicit expression for G; this proof is not so illuminating and requires actually knowing the exact solution] 3. Wilson line with cusp. Use the AdS/CFT duality to compute the strong-coupling behavior of �W [v]�CF T , i.e. the vev of a Wilson loop (in the fundamental) associated to a curve de-scribed by a ’v’ of opening angle θ, in a CFT with a AdS string dual. Show that the renormalized expecation value behaves like ren ln�W [v]� ∼ ln L√4πλ Γ(θ)CF T where Γ is some function of the opening angle which vanishes as θ approaches π (this means that the discontinuity in the line is small). � and L are UV and IR cutoffs on the radial coordinate in AdS (i.e. � < z < L in the coordinates we have been using). 4. Surface gravity. Compute the periodicity of y for which this metric is regular at z = zm (i.e. has no conical deficit): dz2 ds2 = Ω(z) f(z)dy2 + + ds2 f(z) other 2�where f(z) is a function with a first-order zero at z = zm (i.e. ∂zf(zm) = 0 ) and Ω(z) is regular and non-vanishing at z = zm. If we think of y as imaginary time, this periodicity determines the temperature of the black hole, since finite temperature means periodic Euclidean time. a) Specialize your answer to the case of the euclidean Schwarzchild black hole in flat space, for which 2GM f(z) = 1 − , Ω = 1, ds2 = z 2d�x 2 .other z b) Specialize your answer to the case of the euclidean AdS black hole (with planar horizon), for which z4 1 2f(z) ≡ 1 − , Ω = , dsother2 = d�x . 4 2z zm This geometry is also relevant to the model of confinement obtained by com-pactifying a supersymmetric gauge theory on a circle with supersymmetry-breaking (Scherk-Schwarz) boundary conditions. c) Show that you get the same answer by computing the ‘surface gravity’ κ of the horizon (the locus z = zm), which can be defined by 1 acκ2 ≡ 2�aξb�cξd gbdg |z=zm where ξa is the tangent vector to the shrinking circle, ξ = ∂y.


View Full Document

MIT 8 821 - Problem Set 5

Download Problem Set 5
Our administrator received your request to download this document. We will send you the file to your email shortly.
Loading Unlocking...
Login

Join to view Problem Set 5 and access 3M+ class-specific study document.

or
We will never post anything without your permission.
Don't have an account?
Sign Up

Join to view Problem Set 5 2 2 and access 3M+ class-specific study document.

or

By creating an account you agree to our Privacy Policy and Terms Of Use

Already a member?