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  2. Slide 1

    www.damtp.cam.ac.uk/user/examples/A11Lg.pdf
    15 May 2019: Any Beginning in a Quantum Universe? Lorentzian and Euclidean. Gott; Hartle & Hawking. ... Guth, The Inflationary Universe, 2nd edn.( Vintage 1998).  S.W. Hawking and R.
  3. AdSRingsV3

    www.damtp.cam.ac.uk/research/hep/files/conferences/EurostringTalks/Figueras.pdf
    6 Feb 2019: They are topologically spherical [Hawking]. • They rotate rigidly with respect to asymptotic observers [Hawking]. • ... Big black hole. thermal AdS. Phase transition when β l : Hawking-Page Confinement/deconfinement: F O(1) for small T and F ceff
  4. Conformally isometric embeddings and Hawking temperature

    www.damtp.cam.ac.uk/user/md327/dt_haw.pdf
    11 Jul 2019: Classical and Quantum Gravity. PAPER. Conformally isometric embeddings and Hawking temperatureTo cite this article: Maciej Dunajski and Paul Tod 2019 Class. ... Keywords: conformal geometry, Hawking temperature, isometric embeddings. (Some figures may
  5. Cheng.key

    www.damtp.cam.ac.uk/research/hep/files/conferences/EurostringTalks/Cheng.pdf
    6 Feb 2019: Hawking Radiation suggests that black holes are thermodynamical objects. Weakly Coupled Gravitational Theory Black Hole Thermodynamics. ... E >c. 24. c24. < E < 0. A (Hawking-Page) first-order phase transition.
  6. PowerPoint Presentation

    www.damtp.cam.ac.uk/user/examples/A11Le.pdf
    8 May 2019: Hawking, 1975. dE/dt = d(Mc2)/dt = area  aT4  c  M2  M-4 so Lifetime = dt  M2dM  M3.
  7. eurostrings15

    www.damtp.cam.ac.uk/research/hep/files/conferences/EurostringTalks/Mathur.pdf
    6 Feb 2019: Nevertheless, the density of energy quanta remains much larger than that predicted by the Hawking state. ... way to avoid information transfer from right to left throughthe tunneling process of Hawking radiation.
  8. Action Principles

    www.damtp.cam.ac.uk/user/examples/A11Lh.pdf
    22 May 2019: observable. This is why black holes can evaporate. by the Hawking effect.
  9. LargeDUniversal

    www.damtp.cam.ac.uk/research/hep/files/conferences/EurostringTalks/Emparan.pdf
    6 Feb 2019: Finite energy of Hawking radn: 𝑟0 𝐿𝑃𝑙𝑎𝑛𝑐𝑘 𝐷2. Black hole perturbations.
  10. EuroStrings2015.key

    www.damtp.cam.ac.uk/research/hep/files/conferences/EurostringTalks/Dabholkar.pdf
    6 Feb 2019: What is the exact quantum generaliza"on of the celebrated Bekenstein-‐Hawking formula? ... Bekenstein-‐Hawking-‐Wald entropy. ATISH DABHOLKAR QUANTUM ENTROPY OF BLACK HOLES. Compu@ng Quantum Entropy.
  11. 30 Dec 2019: For example, the Gibbons-Hawking metrics [25] give a trivial Einstein–Weyl structure with the maximal symmetrygroup, but the four-metric is in general not so symmetric.

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