Inflationary Cosmology in a non-minimal f (R, T) gravity theory using a RT mixing term

被引:7
作者
Sarkar, Payel [1 ]
Ashmita [1 ]
Das, Prasanta Kumar [1 ]
机构
[1] Birla Inst Technol & Sci Pilani, Dept Phys, KK Birla Goa Campus,NH-17B,Bypass Rd, Zuarinagar 403726, Goa, India
关键词
Inflation; Non-minimal coupling; RT-mixing term; Spectral index parameters; UNIVERSE; STABILITY; FLATNESS; HORIZON; MODELS;
D O I
10.1016/j.dark.2023.101190
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We investigate a class of inflationary models in modified gravity theories which contain a non-minimal coupling between gravity and a scalar field 41 as f (R, T) = R(1 + & alpha; + K4/3T) + K2 & gamma; T where K2 = 8nG where G is Newton's constant. We consider two inflaton potentials of the form (i) V = V0 (1 + ln 41) & lambda;41p and (ii) V0 1+& lambda;41p . For different potential parameters, we have explored the constraints on the modified gravity parameters i.e. (& alpha;, /3, and & gamma;) in the following three cases: (i) /3 = 0, & alpha; = & gamma; = 0, (ii) & alpha; = 0, & gamma; = 0, /3 = 0 and (iii) & gamma; = 0, & alpha; = 0, /3 = 0 for the above two potentials. We find that by the inclusion of RT mixing term, the scalar spectral index ns and tensor-to-scalar ratio r are consistent with the 3 & sigma; limit of the Planck data as well as r < 0.056. & COPY; 2023 Elsevier B.V. All rights reserved.
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页数:8
相关论文
共 73 条
[1]   INDUCED-GRAVITY INFLATION [J].
ACCETTA, FS ;
ZOLLER, DJ ;
TURNER, MS .
PHYSICAL REVIEW D, 1985, 31 (12) :3046-3051
[2]   BICEP2. II. EXPERIMENT AND THREE-YEAR DATA SET [J].
Ade, P. A. R. ;
Aikin, R. W. ;
Amiri, M. ;
Barkats, D. ;
Benton, S. J. ;
Bischoff, C. A. ;
Bock, J. J. ;
Brevik, J. A. ;
Buder, I. ;
Bullock, E. ;
Davis, G. ;
Day, P. K. ;
Dowell, C. D. ;
Duband, L. ;
Filippini, J. P. ;
Fliescher, S. ;
Golwala, S. R. ;
Halpern, M. ;
Hasselfield, M. ;
Hildebrandt, S. R. ;
Hilton, G. C. ;
Irwin, K. D. ;
Karkare, K. S. ;
Kaufman, J. P. ;
Keating, B. G. ;
Kernasovskiy, S. A. ;
Kovac, J. M. ;
Kuo, C. L. ;
Leitch, E. M. ;
Llombart, N. ;
Lueker, M. ;
Netterfield, C. B. ;
Nguyen, H. T. ;
O'Brient, R. ;
Ogburn, R. W. ;
Orlando, A. ;
Pryke, C. ;
Reintsema, C. D. ;
Richter, S. ;
Schwarz, R. ;
Sheehy, C. D. ;
Staniszewski, Z. K. ;
Story, K. T. ;
Sudiwala, R. V. ;
Teply, G. P. ;
Tolan, J. E. ;
Turner, A. D. ;
Vieregg, A. G. ;
Wilson, P. ;
Wong, C. L. .
ASTROPHYSICAL JOURNAL, 2014, 792 (01)
[3]   Planck intermediate results: LVI. Detection of the CMB dipole through modulation of the thermal Sunyaev-Zeldovich effect: Eppur si muove II [J].
Akrami, Y. ;
Ashdown, M. ;
Aumont, J. ;
Baccigalupi, C. ;
Ballardini, M. ;
Banday, A. J. ;
Barreiro, R. B. ;
Bartolo, N. ;
Basak, S. ;
Benabed, K. ;
Bernard, J-P ;
Bersanelli, M. ;
Bielewicz, P. ;
Bond, J. R. ;
Borrill, J. ;
Bouchet, F. R. ;
Burigana, C. ;
Calabrese, E. ;
Cardoso, J-F ;
Casaponsa, B. ;
Chiang, H. C. ;
Combet, C. ;
Contreras, D. ;
Crill, B. P. ;
Cuttaia, F. ;
de Bernardis, P. ;
de Rosa, A. ;
de Zotti, G. ;
Delabrouille, J. ;
Di Valentino, E. ;
Diego, J. M. ;
Dore, O. ;
Douspis, M. ;
Dupac, X. ;
Ensslin, T. A. ;
Eriksen, H. K. ;
Fernandez-Cobos, R. ;
Finelli, F. ;
Frailis, M. ;
Franceschi, E. ;
Frolov, A. ;
Galeotta, S. ;
Galli, S. ;
Ganga, K. ;
Genova-Santos, R. T. ;
Gerbino, M. ;
Gonzalez-Nuevo, J. ;
Gorski, K. M. ;
Gruppuso, A. ;
Gudmundsson, J. E. .
ASTRONOMY & ASTROPHYSICS, 2020, 644
[4]   A designer approach to f(Q) gravity and cosmological implications [J].
Albuquerque, Ines S. ;
Frusciante, Noemi .
PHYSICS OF THE DARK UNIVERSE, 2022, 35
[5]   Dark energy dominance and cosmic acceleration in first-order formalism [J].
Allemandi, G ;
Borowiec, A ;
Francaviglia, M ;
Odintsov, SD .
PHYSICAL REVIEW D, 2005, 72 (06)
[6]  
Ashmita P., arXiv
[7]  
Bahamonde S, 2022, Arxiv, DOI arXiv:2203.00619
[8]  
Baumann D, 2012, Arxiv, DOI arXiv:0907.5424
[9]  
Bazeia D., 2021, EUR PHYS J PLUS, V136, P1
[10]   Extra force in f(R) modified theories of gravity [J].
Bertolami, Orfeu ;
Bohmer, Christian G. ;
Harko, Tiberiu ;
Lobo, Francisco S. N. .
PHYSICAL REVIEW D, 2007, 75 (10)