![]() I compare the result of the holographic approach with the classical-symmetry-algebra-based approach, and I find exact agreements even with the higher-derivative corrections of the gravitational Chern-Simons term. This reproduces, in the limit of a vanishing Einstein-Hilbert term, the recent result about the exotic BTZ black holes, where their masses and angular momenta are completely interchanged and the entropies depend only on the area of the inner horizon. I also find that the new entropy formula agrees with the statistical entropy based on the holographic anomalies for the whole range of the gravitational Chern-Simons coupling. Here I find that there is another entropy formula where the usual Bekenstein-Hawking form dominates the inner-horizon term again, as in the small gravitational Chern-Simons coupling case, such that the second law of thermodynamics can be guaranteed. Zero-Point Mass Entangler: 4: 54.606.666,67: Mid slots Multispectrum Shield Hardener II: 2: 4.295.600,00: Medium Shield Extender II: 3: 2.150. Moreover, this entropy does not agree with the statistical entropy, in contrast to a good agreement for small values of the gravitational Chern-Simons coupling. A basic physical problem of this system is that the form of entropy does not guarantee the second law of thermodynamics, in contrast to the Bekenstein-Hawking entropy. These new frigate wormholes coming with Rhea are all bonused to frigates, making them even easier to run the C1 - C3 sites in AF's. Zero Point Mass Entanglers reduce ship mass by 80 and these reductions stack. You can run C1 - C3 sites (in any type of hole) with relative ease in an Assault Frig. Heavy Interdiction Cruiser (HIC) - Sometimes a hole can end up crit, which means that it isnt safe to put large rolling ships through. But, for large values of the gravitational Chern-Simons coupling where the modification terms dominate the original terms some exotic behaviors occur, like the roles of the mass and angular momentum are interchanged and the entropy depends more on the inner horizon area than the outer one. That would also help drive use of small holes. Recently, the Banados-Teitelboim-Zanelli (BTZ) black hole in the presence of the gravitational Chern-Simons term has been studied, and it is found that the usual thermodynamic quantities, like the black hole mass, angular momentum, and entropy, are modified. There are a few special types of wormhole: one massive wormhole system with stations, Thera, and shattered wormholes, mysterious spaces which cannot have any residents. These solutions are asymptotically AdS in the strongest sense, and correspond to a logarithmic branch of self-dual solutions previously discussed in the literature. ![]() ![]() We study several aspects of the extended thermodynamics of BTZ black holes with thermodynamic mass $$ M=\alpha m \gamma \frac, electrically charged analogues to these solutions exist. In this paper, we present a new semi-quantum private comparison protocol based on entangled states and single particles, which does not require pre-shared keys between the classical users to. ![]()
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