Inflation with a negative cosmological constant

被引:49
作者
Biswas, Tirthabir [1 ]
Mazumdar, Anupam [2 ,3 ]
机构
[1] Penn State Univ, Inst Gravitat & Cosmos, Dept Phys, Davey Lab 104, University Pk, PA 16802 USA
[2] Univ Lancaster, Dept Phys, Lancaster LA1 4YB, England
[3] Niels Bohr Inst, DK-2100 Copenhagen, Denmark
关键词
STRING GAS COSMOLOGY; MODEL HIGGS-BOSON; ENERGY; PERTURBATION; UNIVERSES; ENTROPY;
D O I
10.1103/PhysRevD.80.023519
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We find a unique way of realizing inflation through cyclic phases in a universe with negative vacuum energy. According to the second law of thermodynamics entropy monotonically increases from cycle to cycle, typically by a constant factor. This means that the scale factor at the same energy density in consecutive cycles also increases by a constant factor. If the time period of the oscillations remains approximately constant then this leads to an "overall" exponential growth of the scale factor, mimicking inflation. A graceful exit from this inflationary phase is possible as a dynamical scalar field can take us from the negative to a positive energy vacuum during the last contracting phase.
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页数:9
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