Fluctuation with dust of de Sitter ground state of scalar-tensor gravity-Reference-Cited by-同舟云学术

Fluctuation with dust of de Sitter ground state of scalar-tensor gravity

Published:2014-01-27 Issue:3 Volume:57 Page:411-417
ISSN:1674-7348
Container-title:Science China Physics, Mechanics and Astronomy
language:en
Short-container-title:Sci. China Phys. Mech. Astron.

Author:

Tang YanKe,Zhang HongSheng,Chen ChiYi,Li XinZhou

Publisher

Springer Science and Business Media LLC

Subject

General Physics and Astronomy

Link

http://link.springer.com/content/pdf/10.1007/s11433-014-5395-3.pdf

Reference12 articles.

1. Riess A G, Filippenko A V, Challis P, et al. Observational evidence from supernovae for an accelerating universe and a cosmological constant. Astron J, 1998, 116: 1009–1038; Perlmutter S, Aldering G, Goldhaber G, et al. Measurements of omega and lambda from 42 highredshift supernovae. Astrophys J, 1999, 517: 565–586

2. Copeland E J, Sami M, Tsujikawa S. Dynamics of dark energy. Int J Mod Phys D, 2006, 15: 1753–1935

3. Birrell N, Davies P. Quantum Fields in Curved Space. Cambridge: Cambrige University Press, 1984

4. Nozari K, Shafizadeh S. Non-minimal inflation revisited. Phys Scr, 2010, 82: 015901; Faraoni V. Non-minimal coupling of the scalar field and inflation. Phys Rev D, 1996, 53: 6813–6821; Faraoni V. Does the non-minimal coupling of the scalar field improve or destroy inflation? arXiv:gr-qc/9807066; Okada N, Rehman M U, Shafi Q. Tensor to scalar ratio in non-minimal φ 4 inflation. Phys Rev D, 2010, 82: 043502; Pallis C. Non-minimally gravity-coupled inflationary models. Phys Lett B, 2010, 692: 287–296; Hertzberg M P. On inflation with non-minimal coupling. J High Energy Phys, 2010, 1007: 023; Feng C J, Li X Z. Is non-minimal inflation eternal? Nucl Phys B, 2010, 841: 178–187; Barvinsky A O, Kamenshchik A Y, Kiefer C, et al. Asymptotic freedom in inflationary cosmology with a non-minimally coupled Higgs field. J Cosmol Astropart Phys, 2009, 0912: 003; Hrycyna O, Szydlowski M. Dynamics of extended quintessence on the phase plane. J Cosmol Astropart Phys, 2009, 0904: 026; Park S C. A class of inflation models with non-minimal coupling. J Korean Phys Soc, 2009, 55: 2136; Bauer F, Demir D A. Inflation with non-minimal coupling: Metric vs. palatini formulations. Phys Lett B, 2008, 665: 222–226; Park S C, Yamaguchi S. Inflation by non-minimal coupling. J Cosmol Astropart Phys, 2008, 0808: 009; Nozari K, Sadatian S D. Non-minimal inflation after WMAP3. Mod Phys Lett A, 2008, 23: 2933–2945; Piao Y S, Huang Q G, Zhang X M, et al. Non-minimally coupled tachyon and inflation. Phys Lett B, 2003, 570: 1–4; Hwang J C, Noh H. COBE constraints on inflation models with a massive nonminimal scalar field. Phys Rev D, 1999, 60: 123001

5. Faraoni V. Inflation and quintessence with nonminimal coupling. Phys Rev D, 2000, 62: 023504; Elizalde E, Lopez-Revelles A J. Reconstructing cosmic acceleration from modified and nonminimal gravity: The Yang-Mills case. Phys Rev D, 2010, 82: 063504; Shojai A, Shojai F. Statefinder diagnosis of nearly flat and thawing nonminimal quintessence. Europhys Lett, 2009, 88: 30002; Granda L N, Escobar L D. Holographic dark energy with non-minimal coupling. arXiv: 0910.0515; Setare M R, Vagenas E C. Non-minimal coupling of the phantom field and cosmic acceleration. Astrophys Space Sci, 2010, 330: 145–150; Setare M R, Rozas-Fernandez A. Interacting non-minimally coupled canonical, phantom and quintom models of holographic dark energy in non-flat universe. Int Mod Phys D, 2010, 19: 1987–2002; Gupta G, Saridakis E N, Sen A A. Nonminimal quintessence and phantom with nearly flat potentials. Phys Rev D, 2009, 79: 123013; Nozari K, Davood Sadatian S. Comparison of frames: Jordan vs Einstein frame for a non-minimal dark energy model. Mod Phys Lett A, 2009, 24: 3143–3155; Sen A A, Gupta G, Das S. Non-minimal quintessence with nearly flat potential. J Cosmol Astropart Phys, 2009, 0909: 027; Setare M R, Saridakis E N. Braneworld models with a non-minimally coupled phantom bulk field: A simple way to obtain the −1-crossing at late times. J Cosmol Astropart Phys, 2009, 0903: 002; Hrycyna O, Szydlowski M. Extended quintessence with nonminimally coupled phantom scalar field. Phys Rev D, 2007, 76: 123510; Gonzalez T, Quiros I. Exact models with non-minimal interaction between dark matter and (either phantom or quintessence) dark energy. Class Quantum Gravity, 2008, 25: 175019; Gonzalez T, Leon G, Quiros I. Dynamics of quintessence models of dark energy with exponential coupling to dark matter. Class Quantum Gravity, 2006, 23: 3165–3179; Torres D F. Quintessence, superquintessence, and observable quantities in Brans-Dicke and nonminimally coupled theories. Phys Rev D, 2002, 66: 043522; Sun Z Y, Shen Y G. Phantom cosmology with non-minimally coupled real scalar field. Gen Relativ Gravit, 2005, 37: 243–251.

Cited by 1 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Redshift drift constraints on f(T) gravity;Frontiers of Physics;2015-10