The entropy of Garfinkle-Horne dilaton black hole due to arbitrary spin fields

Using the membrane model which is based on brick wall model, we calculated the free energy and entropy of Garfinkle-Horne dilatonic black hole due to arbitrary spin fields. The result shows that the entropy of scalar field and the entropy of Fermionic field have similar formulas. There is only a coefficient between them.     

Note on the Constraint on Modified Energy-Momentum Relation

Quantum gravity can modify the usual energy-momentum dispersion relation. We provide evidence for the argument that the modified dispersion relation is constrained by the black hole thermodynamics, for consistency of quantum gravity.     

Entropy in the NUT—Kerr—Newman Black Holes in the Background of de Sitter Spacetime

We calculate the entropy of the fermion field in the NUT-Kerr-Newman black holes in the background of the de Sitter spacetime by using the improved brick-wall method and the membrane model.Here the Euler characteristic of the black holes is over two.The results show that,as the cut-off is properly chosen,the entropy in the black hole satisfies the Bekenstein-Hawking area law.     

三维BTZ黑洞的熵

计算了三维BTZ黑洞时空背景下标量场和中微子场的熵. 考虑到统计物理, 我们建议对于Boson子不考虑超辐射模式(Fermi场不表现超辐射). 事实上, 无论是Boson子场还是Fermi子场, 其非超辐射模式刚好给出面积熵. 结果表明, 中微子场的熵是Boson子场熵的3/2倍.     

有限温度下的复标量场的虫洞

本文讨论了有限温度下的具有自发对称破缺的耦合标量场的虫洞,发现对于Coleman-Lee虫洞温度影响是重要的.这种类型的虫洞能够存在于0≤T?M_P的区域中.     

Extra Dimensions and Vacuum Dark Energy Models

The role of vacuum energy or cosmological constant in cosmology is discussed in a kind of nontrivial higherdimensional model. Under the framework of Einstein‘s gravity, we obtain the corresponding equations of motion and find that the cosmological constant and vacuum energy in the full regime does not drive its acceleration, but decelerates the expansion of the universe. The dimension of space is required to be n = 3 if we regard vacuum energy or cosmological constant as the candidate to drive the accelerated expansion of the universe.