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On the stability of string-hole gas

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arxiv 2308.16764 v2 pith:BH7LJHT3 submitted 2023-08-31 hep-th astro-ph.COgr-qc

classification hep-thastro-ph.COgr-qc
keywords string-holeviscositystabilityactionalphaprimesolutionterm
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abstract

Focusing on a string-hole gas within the pre-big bang scenario, we study the stability of its solutions in the phase space. We firstly extend the analysis present in the literature relaxing the ideal-gas properties of the string-hole gas, taking into account a (bulk-)viscosity term. Then we consider the case of a theory described by a complete O(d,d)-invariant action up to all orders in $\alpha^{\prime}$-corrections (the Hohm-Zwiebach action), studying the stability of the string-hole gas solution with or without the introduction of the viscosity term. Furthermore, the bulk viscosity is also considered for two different first order $\alpha^{\prime}$-corrected actions: the Gasperini-Maggiore-Veneziano-action and the Meissner-action. The results obtained show how the viscosity can help to stabilize the string-hole gas solution, obtaining constraints on the equation of state of the gas.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Viscosity in Isotropic Cosmological Backgrounds in General Relativity and Starobinsky Gravity

    gr-qc 2025-06 conditional novelty 6.0 of 10

    Shear viscosity does not affect the background expansion or the electromagnetic luminosity distance in isotropic cosmologies with a comoving fluid, also in Starobinsky gravity.

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