de Sitter space and Holography

de Sitter space and Holography de Sitter space and Holography

hep.physics.uoc.gr
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13.07.2015 Views

• One can always decompose the metric h µν on the equaltime surfaces as followsh νν dx µ dx ν = N ρ dρ 2 + σ ab (dφ a + U a dρ)(dφ b + U b dρ)where φ a are angular variables parameterizing closed surfaces.• Suppose the boundary has an isometry generated by aKilling vector ξ µ . One can show that T µν ξ ν is divergencelessand therefore we can define conserved charge associated to ξ µ .• Consider n µ be the unit normal on a surface of fixed ρ.Then the conserved charge is defined∮Q = d d−2 φ √ σn µ ξ ν T µνΣPhysically this means that a collection of observers on thehypersurface whose metric is h µν would all observe the samevalue of Q provided this surface had an isometry generated byξ µ .Since there is no globally timelike Killing vector, it is difficultto see how the mass can be defined in dS space. There ishowever an proposal for this using the above construction.Consider the case where ρ is the coordinate associated withthe asymptotic Killing vector that is timelike inside the staticpatch but spacelike at I − .36

The mass of an asymptotically dS space is∮M = d d−2 φ √ σN ρ n µ n ν T µνΣOne may also define momenta as∮J a =Σd d−2 φ √ σσ ab n ν T bν 37

• One can always <strong>de</strong>compose the metric h µν on the equaltime surfaces as followsh νν dx µ dx ν = N ρ dρ 2 + σ ab (dφ a + U a dρ)(dφ b + U b dρ)where φ a are angular variables parameterizing closed surfaces.• Suppose the boundary has an isometry generated by aKilling vector ξ µ . One can show that T µν ξ ν is divergenceless<strong>and</strong> therefore we can <strong>de</strong>fine conserved charge associated to ξ µ .• Consi<strong>de</strong>r n µ be the unit normal on a surface of fixed ρ.Then the conserved charge is <strong>de</strong>fined∮Q = d d−2 φ √ σn µ ξ ν T µνΣPhysically this means that a collection of observers on thehypersurface whose metric is h µν would all observe the samevalue of Q provi<strong>de</strong>d this surface had an isometry generated byξ µ .Since there is no globally timelike Killing vector, it is difficultto see how the mass can be <strong>de</strong>fined in dS <strong>space</strong>. There ishowever an proposal for this using the above construction.Consi<strong>de</strong>r the case where ρ is the coordinate associated withthe asymptotic Killing vector that is timelike insi<strong>de</strong> the staticpatch but <strong>space</strong>like at I − .36

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