BOUNDS ON f(G) GRAVITY FROM ENERGY CONDITIONS

DOI10.1142/S0217732310033384zbMath1194.83125OpenAlexW2122926635MaRDI QIDQ3590681

Puxun Wu, Hong Wei Yu

Publication date: 13 September 2010

Published in: Modern Physics Letters A (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1142/s0217732310033384

zbMATH Keywords

energy conditionmodified gravitycosmic accelerating expansion

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)

Cites Work

• A note on the viability of Gauss-Bonnet cosmology
• Modified Gauss-Bonnet theory as gravitational alternative for dark energy
• Constraining \(f(R)\) theories with the energy conditions
• Cosmology and astrophysical constraints of Gauss-Bonnet dark energy
• Ghost conditions for Gauss-Bonnet cosmologies
• Cosmological scaling solutions in generalised Gauss-Bonnet gravity theories
• <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math>theories of gravity
• ENERGY CONDITIONS IN f(R) GRAVITY AND BRANS–DICKE THEORIES
• INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY
• From Inflation to Dark Energy in the Non-Minimal Modified Gravity
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae
• Type Ia Supernova Discoveries atz> 1 from theHubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution

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