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Critical exponents of gravity with quantum perturbations Center - - PowerPoint PPT Presentation

Critical exponents of gravity with quantum perturbations Center for Astrophysics, Shanghai Normal University Prime ref: H Zhang ( ), X Li, arXiv:1208.0106 Outline 1. Introduction to thermo dynamical gravity 2.


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Critical exponents of gravity with quantum perturbations

张宏升

Center for Astrophysics, Shanghai Normal University

Prime ref: H Zhang (张宏升), X Li, arXiv:1208.0106

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Outline

  • 1. Introduction to thermo dynamical gravity
  • 2. Critical exponents of RN-AdS black hole
  • 3. Quantum perturbations included

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Introduction to thermo dynamical gravity

  • Temperature: 1/(8πM)
  • Entropy: A/4
  • Energy: M
  • Event horizon: r+=2M, A=4 πr+

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Van der Waals-Maxwell gas-liquid system

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Equation of state Critical point

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Critical isotherm

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Critical isotherm

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  • Critical exponents of RN black

hole

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RN-AdS space time

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Entropy, temperature, and potential

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Equation of state of RN-AdS

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Critical point

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Critical exponents

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Definition

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N-dimensional case

  • For n-dim RN-AdS black hole, the critical

exponents take the same values as that of 4- dim case, ie, C Niu, Y Tian, X Wu, Phys.Rev.D85:024017,2012

  • This is a distinctive property of MFT( mean

field theory).

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  • Quantum perturbations

included

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Temperature correction of Hawking radiation

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This equation includes the total effects of the quantum perturbations to all orders.

  • R. Banerjee and B. R. Majhi, JHEP 0806, 095 (2008)
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Critical point for corrected temperature

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Values of critical quantities

  • A special method to solve the above equation.
  • The essential condition is that two roots of

degenerates to one. Under this condition, and

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The simplified equation

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The simplified equation

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8 variables in the above set

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The critical isotherm

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Result of critical exponents

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Physical interpretations

  • For ordinary matter, MFT and RGT present different critical
  • exponents. Theoretically, MFT omits the perturbations

around the critical point, while RGT carefully considers the perturbation effects at the critical point. In RGT, the whole system at the critical point is length scale free, that is, there is no special length scale in this system. In a gravity system, there is an inherent length scale G^(-1/2), which makes the RGT cannot do its work in a gravity system. A popular result is that the G^(-1/2) with a length scale hinders us to renormalize gravity. Here it hinders us to apply RGT in gravity, which makes the perturbed gravity and unperturbed gravity share the same critical exponents, though the perturbation shifts the critical point.

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  • Thank you for your

attention.

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