The Casimir energy of massive scalar field with hybrid （Diriehlet-Neumann） boundary condition is calculated. In order to regularize the model, the typical methods named as mode summation method and Green＇s function...The Casimir energy of massive scalar field with hybrid （Diriehlet-Neumann） boundary condition is calculated. In order to regularize the model, the typical methods named as mode summation method and Green＇s function method are used respectively. It is found that the regularized zero-point energy density depends on the scalar field＇s mass. When the field is massless, the result is consistent with previous literatures.展开更多
We study the scalar and fermionic retarded Green＇s function on the background with hyperscMing violation by means of the prescriptions proposed in [J. High Eergy Phys. 09 （2002） 042; Fortsch. Phys. 57 （2009） 367]...We study the scalar and fermionic retarded Green＇s function on the background with hyperscMing violation by means of the prescriptions proposed in [J. High Eergy Phys. 09 （2002） 042; Fortsch. Phys. 57 （2009） 367]. For scalar field, we consider both massless and massive cases, and for spinor field, we further calculate the finite temperature correlator with the black hole background.展开更多
基金supported by National Natural Science Foundation of China under Grant Nos.10773002 and 10875012the National Fundamental Research Program of China under Grant No.2003CB716302
文摘The Casimir energy of massive scalar field with hybrid （Diriehlet-Neumann） boundary condition is calculated. In order to regularize the model, the typical methods named as mode summation method and Green＇s function method are used respectively. It is found that the regularized zero-point energy density depends on the scalar field＇s mass. When the field is massless, the result is consistent with previous literatures.
文摘We study the scalar and fermionic retarded Green＇s function on the background with hyperscMing violation by means of the prescriptions proposed in [J. High Eergy Phys. 09 （2002） 042; Fortsch. Phys. 57 （2009） 367]. For scalar field, we consider both massless and massive cases, and for spinor field, we further calculate the finite temperature correlator with the black hole background.
