Presentation is loading. Please wait.

Presentation is loading. Please wait.

Area scaling from entanglement in flat space quantum field theory Introduction Area scaling of quantum fluctuations Unruh radiation and Holography.

Similar presentations


Presentation on theme: "Area scaling from entanglement in flat space quantum field theory Introduction Area scaling of quantum fluctuations Unruh radiation and Holography."— Presentation transcript:

1 Area scaling from entanglement in flat space quantum field theory Introduction Area scaling of quantum fluctuations Unruh radiation and Holography

2 Black hole thermodynamics J. Beckenstein (1973) S. Hawking (1975) S  A THTH S = ¼ A

3 An ‘artificial’ horizon. V V in out

4 Entropy: S in =Tr(  in ln  in ) S in =S out Srednicki (1993)

5 Entanglement entropy of a sphere out in Entropy R2R2 Srednicki (1993)

6 Other Thermodynamic quantities Heat capacity: More generally:  A ? ?

7 A different viewpoint in out = No accessRestricted measurements

8 Area scaling of fluctuations R. Brustein and A.Y., (2004)  O a V1 O b V2  V1V1 Assumptions: V2V2  O a V1 2 

9 Area scaling of correlation functions  O a V1 O b V2  =  V1  V2  O a (x) O b (y)  d d x d d y =  V1  V2 F ab (|x-y|) d d x d d y =  D(  ) F ab (  ) d  D(  )=  V  V  (  x  y  ) d d x d d y Geometric term: Operator dependent term =  D(  )  2 g(  ) d  = -  ∂  (D(  )/  d-1 )  d-1 ∂  g(  ) d 

10 Geometric term D(  )=  V1  V2  (  x  y  ) d d x d d y V1V1 V2V2 =    (  r) d d r d d R  d d R  A  2 )  (  r) d d r   d-1 +O(  d ) D(  )=C 2 A  d + O(  d+1 )

11 Geometric term D(  )=    (  r) d d r d d R  d d R  V + A  2 )  (  r) d d r   d-1 +O(  d ) D(  )=C 1 V  d-1 ± C 2 A  d + O(  d+1 ) V 1 =V 2

12 Area scaling of correlation functions  O a V1 O b V2  =  V1  V2  O a (x) O b (y)  d d x d d y =  V1  V2 F ab (|x-y|) d d x d d y =  D(  ) F ab (  ) d  =  D(  )  2 g(  ) d   ∂  (D(  )/  d-1 )   = -  ∂  (D(  )/  d-1 )  d-1 ∂  g(  ) d  UV cuttoff at  ~1/  D(  )=C 1 V  d-1 + C 2 A  d + O(  d+1 )  A

13 Energy fluctuations

14 Intermediate summary V V Tr(  in O V ) Tr(  in O V 2 )

15 Finding  in  (x,0)=  (x) x t  ’(x)  ’’(x) Tr out  (  ’  ’’   in (  ’ in,  ’’ in ) =  in  ’ in  ’’ in    Exp[-S E ] D   (x,0 + ) =  ’ in (x)  (x,0 - ) =  ’’ in (x)  (x,0 + ) =  ’ in (x)  out (x)  (x,0 - ) =  ’’ in (x)  out (x)   Exp[-S E ] D  D  out  ’’ in (x)  ’ in (x)  (x,0 + )=  ’(x)  (x,0 - )=  ’’(x)  (x,0 + )=  ’(x)  (x,0 - )=  ’’(x)

16 Finding rho x t  ’ in (x)  ’’ in (x)  in  ’ in  ’’ in    Exp[-S E ] D   (x,0 + ) =  ’ in (x)  (x,0 - ) =  ’’ in (x)  ’| e -  K |  ’’  Kabbat & Strassler (1994)

17 Rindler space (Rindler 1966) ds 2 = -dt 2 +dx 2 +  dx i 2 ds 2 = -a 2  2 d  2 +d  2 +  dx i 2 t=  /a sinh(a  ) x=  /a cosh(a  ) Acceleration = a/  Proper time =  x t  = const  =const H R = K x

18 Unruh Radiation (Unruh, 1976) x t ds 2 = -a 2  2 d  2 +d  2 +  dx i 2  = 0 a  ≈ a  +i2  Avoid a conical singularity Periodicity of Greens functions Radiation at temperature  0 = 2  /a  R =  e -  H R  =  e -  K  =  in

19 Schematic picture VEVs in V of Minkowski space VV Observer in Minkowski space with d.o.f restricted to V Canonical ensemble in Rindler space (if V is half of space) Tr(  in O V ) = Tr(  R O V ) =

20 Other shapes R. Brustein and A.Y., (2003)  in  ’ in  ’’ in    Exp[-S E ] D   (x,0 + ) =  ’ in (x)  (x,0 - ) =  ’’ in (x) x t  ’’ in( x)  ’ in( x)   =  ’ in |e -  H 0 |  ’’ out  d/dt H 0 = 0 S E =  0  H 0 dt  (x,t),  (x,t), +B.C. H 0 =K, in={x|x>0}

21 Evidence for bulk-boundary correspondence V1V1  O V1 O V2  A 1  A 2 OV1OV2OV1OV2 V2V2 OV1OV2OV1OV2  V1 V2 V1 V2  O V1 O V2  -  O V 1  O V2  Pos. of V 2 R. Brustein D. Oaknin, and A.Y., (2003)

22 A working example Large N limit R. Brustein and A.Y., (2003)

23 Summary V Area scaling of Fluctuations due to entanglement Unruh radiation and Area dependent thermodynamics A Boundary theory for fluctuations Statistical ensemble due to restriction of d.o.f V A Minkowski observer restricted to part of space will observe: Radiation. Area scaling of thermodynamic quantities. Bulk boundary correspondence*.

24 Speculations Theory with horizon (AdS, dS, Schwarzschild) A Boundary theory for fluctuations V Area scaling of Fluctuations due to entanglement Statistical ensemble due to restriction of d.o.f V ??? Israel (1976) Maldacena (2001)

25 Fin


Download ppt "Area scaling from entanglement in flat space quantum field theory Introduction Area scaling of quantum fluctuations Unruh radiation and Holography."

Similar presentations


Ads by Google