::: Hot Negro B*tches w/ STDs :::

::: Hot Negro B*tches w/ STDs :::
                - or -
      bLaCK hOlE eNtrOpY!

This one just in from Dr. Emmet "Doc" Brown:

   http://en.wikipedia.org/wiki/Back_to_the_Future
   <sarfatti@pacbell.net>

[It's some VERY SMART stuff intended only for the High Foreheads w/
Coke-Bottle-Bottom Glasses crowd.  Note: do NOT confuse Area Flux
Operators [i.e. dTheta/\dPhi] with Sarfatti's Top Secret Flux
Capacitors!]

Black hole entropy and SU(2) Chern-Simons theory
=====================================
Jonathan Engle, Karim Noui, Alejandro Perez
(Submitted on 19 May 2009)

We show that the isolated horizon boundary condition can be treated in
a manifestly SU(2) invariant manner. The symplectic structure of
gravity with the isolated horizon boundary condition has an SU(2)
Chern-Simons symplectic structure contribution at the horizon with
level k=a_H/ (4\pi \beta \ell^2_p). Upon quantization, state counting
is expressed in terms of the dimension of Chern-Simons Hilbert spaces
on a sphere with marked points (defects). In the large black hole
limit quantum horizon degrees of freedom can be modelled by a single
intertwiner. The coupling constant of the defects with the Chern
Simons theory on the horizon is precisely given by the ratio of the
area contribution of the defect to the macroscopic area a_H, namely
\lambda= 16\pi^2 \beta \ell^2_p (j(j+1))^(1/2)/a_H.

Comments: 4 pages, 1 figure
Subjects: General Relativity and Quantum Cosmology (gr-qc)
Cite as: arXiv:0905.3168v1 [gr-qc]

Area flux operator is dTheta/\dPhi
 arXiv:0905.3465 [ps, pdf, other]

Flux-area operator and black hole entropy
J. Fernando Barbero G., Jerzy Lewandowski, Eduardo J. S. Villase�or
Comments: 25 pages
Subjects: General Relativity and Quantum Cosmology (gr-qc)

We show that, for space-times with inner boundaries, there exists a
natural area operator different from the standard one used in loop
quantum gravity. This new flux-area operator has equidistant
eigenvalues. We discuss the consequences of substituting the standard
area operator in the Ashtekar-Baez-Corichi-Krasnov definition of black
hole entropy by the new one. Our choice simplifies the definition of
the entropy and allows us to consider only those areas that coincide
with the one defined by the value of the level of the Chern-Simons
theory describing the horizon degrees of freedom. We give a
prescription to count the number of relevant horizon states by using
spin components and obtain exact expressions for the black hole
entropy. Finally we derive its asymptotic behavior, discuss several
issues related to the compatibility of our results with the Bekenstein-
Hawking area law and the relation with Schwarzschild quasi-normal
modes.

BELIEVE IT OR NOT!

Dr. Blue Resonant Human, Ph.D.