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RECENT POSTS IN THIS TOPIC

SHANKARANARAYANAN S: on 3/8/17 at 18:02pm UTC, wrote Hi, Thanks for your message. We will send our comments to your essay asap....

SHANKARANARAYANAN S: on 3/8/17 at 17:59pm UTC, wrote Hi Steve, Thanks for your kind message. Best, Shanki

Joe Fisher: on 3/8/17 at 17:20pm UTC, wrote Dear Swastik Bhattacharya and S. Shankaranarayanan, Please excuse me...

Satyavarapu Gupta: on 3/8/17 at 15:50pm UTC, wrote Nice essay Bhattacharya, Shankaranarayanan , Your essay is basically about...

Steve Dufourny: on 3/8/17 at 11:33am UTC, wrote Hello to both of you, I liked a lot your papper and how you analyse these...

SHANKARANARAYANAN S: on 3/6/17 at 8:38am UTC, wrote Dear Dr. Akerlund, Thanks for the comments. Sorry for being brief with the...

james akerlund: on 3/6/17 at 5:13am UTC, wrote I read your interesting article, but it seems to me one of two things...

SHANKARANARAYANAN S: on 3/6/17 at 2:15am UTC, wrote Dear Prof. Stoica, Thank you for your detailed reply. It is very much...


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FQXi FORUM
March 28, 2017

CATEGORY: Wandering Towards a Goal Essay Contest (2016-2017) [back]
TOPIC: Does the future determine the dynamics of horizons in quantum gravity? by Shankaranarayanan S and Swastik Bhattacharya [refresh]
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This essay's rating: Community = 4.3; Public = 2.0


Author SHANKARANARAYANAN S wrote on Mar. 3, 2017 @ 16:02 GMT
Essay Abstract

General Relativity predicts the existence of black-holes. Access to the complete space-time manifold is required to describe black-holes. This strange feature necessitates that black-hole dynamics is specified by future or teleological boundary condition. Here we demonstrate that the statistical mechanical description of black-holes, as required by the laws of black-hole thermodynamics, also requires teleological boundary condition. It is known for three decades that the Einstein's equations when projected on space-time horizons resemble Navier-Stokes equation of a fluid. Within this paradigm, we show that the specific heat and the coefficient of bulk viscosity of the horizon-fluid are negative only if the teleological boundary condition is taken into account. We argue that in quantum theory of gravity, the future boundary condition plays a crucial role and discuss its implications.

Author Bio

Shankaranarayanan obtained his Ph.D. in 2002 from IUCAA, Pune, India. After postdoctoral work at the University of Azores, ICTP-Trieste, Italy and Albert Einstein Institute-Golm, Germany; he was a Marie Curie Fellow at the ICG, Portsmouth, UK. Since 2009, he is a faculty at ISER-Thiruvananthapuram and heads Max Planck Partner Group on Cosmology and Gravity. His interests is Early-Universe Cosmology and Gravity. Bhattacharya did his PhD from TIFR, Mumbai, India. His current research interests are understanding the physics of black holes and exploring the challenges in putting together the Quantum theory and Gravity. Currently he is a postdoctoral fellow at IISER-Thiruvananthapuram.

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Cristinel Stoica wrote on Mar. 5, 2017 @ 07:44 GMT
Dear Swastik Bhattacharya and S. Shankaranarayanan,

Your essay is well-written and very interesting. The fluid approach to the black hole thermodynamics has relevant implications, not only to the problem itself, but also to the utility of future boundary conditions. Indeed, it appears that not only the definition of the horizon requires such a view, but also the statistical descriptions of black hole entropy and temperature. I think your approach and the corresponding paradigm which relates the projection of Einstein equation on the horizon to the Navier-Stokes equation of a fluid is very promising to say the least, since it allows the study of the black hole thermodynamics without having to assume much about the quantum gravity level and the Plank scale. So whatever these may be, I think some of the fundamental properties can already be captured in this method.

Best regards,

Cristi Stoica

The Tablet of the Metalaw

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Author SHANKARANARAYANAN S replied on Mar. 6, 2017 @ 02:15 GMT
Dear Prof. Stoica,

Thank you for your detailed reply. It is very much appreciated.

Best,

Shanki




james r. akerlund wrote on Mar. 6, 2017 @ 05:13 GMT
I read your interesting article, but it seems to me one of two things occurred. You cut it to fit the FQXi page requirements and that made it hard to read, or you wrote it for a very specific audience that is understanding of the finer points you bring up. To give you and example. You give a bunch of equations, but most do not include definitions of the variables. On page 9 of your article you give the equation P = nk_BT n = N/V. I'm guessing k_B is Boltzmann's constant, T is temperature, but I'm not sure about N and V. If you have a longer version of this article somewhere on the web I might be interested in reading it to see the finer points that I am missing in this article.

Anyway, good luck in the contest.

Jim Akerlund

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Author SHANKARANARAYANAN S replied on Mar. 6, 2017 @ 08:38 GMT
Dear Dr. Akerlund,

Thanks for the comments. Sorry for being brief with the defintions. You guess about $k_B$, $T$ is correct. $N$ is the number of particles and $V$ is the volume.

You can look our earlier works that are in the arxiv:

https://arxiv.org/abs/1702.03682

https://arxiv.org/abs/1607.0
6222

https://arxiv.org/abs/1512.03680

Thanks, once again, for your comments.

Best,

Shanki




Steve Dufourny wrote on Mar. 8, 2017 @ 11:33 GMT
Hello to both of you,

I liked a lot your papper and how you analyse these BHs and the horizons.The BEC also seems very relevant.I consider that dark matter, gravitation and BHs are in the cold.This zero absolute seems very relevant considering the equilibrium between gravity and electromagntism.Thanks for sharing your works and good luck in this contest.You are going to be well ranked.

Regards

report post as inappropriate

Author SHANKARANARAYANAN S replied on Mar. 8, 2017 @ 17:59 GMT
Hi Steve,

Thanks for your kind message.

Best,

Shanki




Satyavarapu Naga Parameswara Gupta wrote on Mar. 8, 2017 @ 15:50 GMT
Nice essay Bhattacharya, Shankaranarayanan ,

Your essay is basically about Blackholes, Bigbang and CMB etc… As for Bigbang and Blackholes are mathematical singularities. As for CMB, they have not accounted for the microwave radiation emitted from Galaxies, Globular clusters and stars etc… see the essay on CMB in previous FQXi... There was no provision to eliminate this radiation in the...

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Joe Fisher wrote on Mar. 8, 2017 @ 17:20 GMT
Dear Swastik Bhattacharya and S. Shankaranarayanan,

Please excuse me for I have no intention of disparaging in any way any part of your essay.

I merely wish to point out that “Everything should be made as simple as possible, but not simpler.” Albert Einstein (1879 - 1955) Physicist & Nobel Laureate.

Only nature could produce a reality so simple, a single cell amoeba could deal with it.

The real Universe must consist only of one unified visible infinite physical surface occurring in one infinite dimension, that am always illuminated by infinite non-surface light.

A more detailed explanation of natural reality can be found in my essay, SCORE ONE FOR SIMPLICITY. I do hope that you will read my essay and perhaps comment on its merit.

P.S. My essay, THE SIMPLEST UNIVERSE was sent out for review by the editor of the Indian Institute Journal of Current Science on December 28, 2016. The email address for inquiries at the site cannot be accessed by my rr email server. Could you possibly advise me as to how I might find out about the delay?

Joe Fisher, Realist

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Author SHANKARANARAYANAN S replied on Mar. 8, 2017 @ 18:02 GMT
Hi,

Thanks for your message. We will send our comments to your essay asap.

Regarding Current Science: We are part of a different organization and we do not

know about the Procedures followed in Current Science.

Thanks,

Shanki




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