UNIFIED DARK MATTER IN SCALAR FIELD COSMOLOGIES
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Publication:3509740
DOI10.1142/S0217732307025893zbMath1152.83028arXivastro-ph/0703259OpenAlexW3098414429WikidataQ59274621 ScholiaQ59274621MaRDI QIDQ3509740
Daniele Bertacca, Sabino Matarrese, M. Pietroni
Publication date: 2 July 2008
Published in: Modern Physics Letters A (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/astro-ph/0703259
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Cites Work
- Unification of dark matter and dark energy: the inhomogeneous Chaplygin gas
- No-Go Theorem for<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>k</mml:mi></mml:math>-Essence Dark Energy
- DYNAMICS OF DARK ENERGY
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
- Cosmological Imprint of an Energy Component with General Equation of State
- The cosmological constant problem
- Cosmological dynamics of the tachyon with an inverse power-law potential
- \(k\)-inflation
- Perturbations in \(k\)-inflation
- An alternative to quintessence
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