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A note on vacuum energy from the de Sitter spectrum

Kostyantyn Ropotenko

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COMMENTS, REPLIES AND NOTES

It is shown that a well-known relation between entropy of a system and its energy spectrum being applied to the early universe determines the present vacuum energy and the time scale on which this energy can manifest itself. Given the present vacuum energy, the relation imposes a constraint on the initial inflationary state.


PACS

98.80.Cq Particle-theory and field-theory models of the early Universe (including cosmic pancakes, cosmic strings, chaotic phenomena, inflationary universe, etc.)

98.80.Es Observational cosmology (including Hubble constant, distance scale, cosmological constant, early Universe, etc)

95.30.Tg Thermodynamic processes, conduction, convection, equations of state

MSC

83F05 Cosmology

Subjects

Gravitation and cosmology

Astrophysics and astroparticles

Dates

Issue 22 (21 November 2007)

Received 9 August 2007

Published 6 November 2007



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