2003
DOI: 10.1103/physrevd.67.124003
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Regular cosmological bouncing solutions in low energy effective action from string theories

Abstract: The possibility of obtaining singularity free cosmological solutions in four dimensional effective actions motivated by string theory is investigated. In these effective actions, in addition to the Einstein-Hilbert term, the dilatonic and the axionic fields are also considered as well as terms coming from the Ramond-Ramond sector. A radiation fluid is coupled to the field equations, which appears as a consequence of the Maxwellian terms in the Ramond-Ramond sector. Singularity free bouncing solutions in which … Show more

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Cited by 44 publications
(52 citation statements)
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References 30 publications
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“…The features we have discussed can be seen in figure 6, which shows a numerical solution to the combined gravitational equations of motion (6), (8) and the strongcoupling Boltzmann equations (31), (32). The matter energy E has plateaus which 11 Note that no real temperature is dropping here since during the Hagedorn phase the temperature is constant at T H .…”
Section: Shrinking Cyclesmentioning
confidence: 92%
See 2 more Smart Citations
“…The features we have discussed can be seen in figure 6, which shows a numerical solution to the combined gravitational equations of motion (6), (8) and the strongcoupling Boltzmann equations (31), (32). The matter energy E has plateaus which 11 Note that no real temperature is dropping here since during the Hagedorn phase the temperature is constant at T H .…”
Section: Shrinking Cyclesmentioning
confidence: 92%
“…Our work provides a simple string-inspired mechanism for obtaining bouncing and cyclic cosmologies. For other studies in this direction see [8,9,10].…”
Section: Bouncing and Cyclic Cosmologiesmentioning
confidence: 99%
See 1 more Smart Citation
“…However, particular cases can be explicitly solved. The solutions without the moduli fields were found in reference [15]; the main scenarios for this case will be reviewed below. The equations, in the presence of moduli fields, but in the absence of the Ramond-Ramond (RR) term, will be solved for two main cases: in the absence of the axion field, and in the presence of the axion field.…”
Section: Regular Cosmological Solutionsmentioning
confidence: 99%
“…This means that in the Einstein frame, negative energies are present. The flat solutions of interest were obtained in reference [15]. They are the following:…”
Section: Solutions In Absence Of the Moduli Fieldsmentioning
confidence: 99%