Tunneling in Λ decaying cosmologies and the cosmological constant problem -: art. no. 063514.

被引:0
作者
Jafarizadeh, MA [1 ]
Darabi, F
Rezaei-Aghdam, A
Rastegar, AR
机构
[1] Tabriz Univ, Dept Theoret Phys, Tabriz 51664, Iran
[2] Inst Studies Theoret Phys & Math, Tehran 193951795, Iran
[3] Shahid Beheshti Univ, Dept Phys, Tehran 19839, Iran
[4] Tarbiyat Moallem Univ, Dept Phys, Tabriz, Iran
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中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The tunneling rate, with an exact prefactor, is calculated to first order in (h) over bar for an empty closed Friedmann-Robertson-Walker universe with a decaying cosmological term Lambda similar to R-m (R is the scale factor and m is a parameter 0 less than or equal to m less than or equal to 2). This model is equivalent to a cosmology with the equation of state p(chi)=(m/3-1)rho(chi). The calculations are performed by applying the dilute-instanton approximation on the corresponding Duru-Kleinert path integral. It is shown that the highest tunneling rate occurs for m = 2 corresponding to the cosmic string matter universe. The most probable cosmological term obtained, such as the one obtained by Strominger, accounts for a possible solution to the cosmological constant problem. [S0556-2821(99)03016-7].
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