Friedmann–Robertson–Walker accelerating Universe with interactive dark energy (original) (raw)
Abstract
We have developed an accelerating cosmological model for the present universe which is phantom for the period (0 ≤ z ≤ 1.99) and quintessence phase for (1.99 ≤ z ≤ 2.0315). The universe is assumed to be filled with barotropic and dark energy(DE) perfect fluid in which DE interact with matter. For a deceleration parameter(DP) having decelerating-accelerating transition phase of universe, we assume hybrid expansion law for scale factor. The transition red shift for the model is obtained as zt = 0.956. The model satisfies current observational constraints.
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References (82)
- S. Perlmutter et al., Nature 391, 51 (1998).
- S. Perlmutter et al., Astrophys. J. 517, 5 (1999).
- A. G. Riess et al., Astron. J. 116, 1009 (1998).
- J. L. Tonry et al., Astrophys. J. 594, 1 (2003).
- A. Clocchiatti et al., Astrophys. J. 642, 1 (2006).
- P. de Bernardis et al., Nature 404, 955 (2000).
- S. Hanany et al., Astrophys. J. 493, L53 (2000).
- D. N. Spergel et al., Astrophys. J. Suppl. 148, 175 (2003).
- M. Tegmark et al, Phys. Rev. D 69, 103501 (2004).
- U. Seljak et al., Phys. Rev. D 71, 103515 (2005).
- J. K. Adelman-McCarthy et al., Astrophys. J. Suppl. 162, 38 (2006).
- C. L. Bennett et al., Astrophys. J. Suppl. 148 1 (2003).
- S. W. Allen et al., Mon. Not. R. Astron. Soc. 353, 457 (2004).
- N. Suzuki et al., Astrophys. J. 746, 85 (2011).
- T. Delubac et al., Astron. Astrophys. 574, A59 (2015).
- C. Blake et al., Mon. Not. R. Astron. Soc. 425, 405 (2012).
- P. A. R. Ade et al., Astron. Astrophys. 594. A14 (2016).
- E. J. Copeland et al., Int. J. Mod. Phys. D 15, 1753 (2006).
- Ø. Grøn and S. Hervik, Einstein's general theory of relativity with modern applications in cosmology, Springer Publication, (2007).
- S. Weinberg, Rev. Mod. Phys. 61, 1 (1989).
- H. Amirhashchi, A. Pradhan and B. Saha, Chin. Phys. Lett. 28 039801(2011).
- H. Amirhashchi ,A. Pradhan and H. Zainuddin, Int. J. Theor. Phys. 50, 3529( 2011)
- A. Pradhan , H. Amirhashchi and B. Saha, Astrophys. Space Sci. 333, 343(2011)
- B. Saha, H. Amirhashch and A. Pradhan, Astrophys. Space Sci. 342, 257(2012)
- A. Pradhan, Indian J. Phys. 88, 215( 2014)
- S. Kumar, Astrophys. Space Sci. 332, 449(2011)
- X.F. Zhang and H. H. Liu, Chin. Phys. Lett. 26, 109803 ( 2009)
- N. M. Liang, C.J. Gao and S.N. Zhang, Chin. Phys. Lett. 26, 069501( 2009)
- C. Wang, Y.B. Wu and F. Liu, Chin. Phys. Lett. 26, 029801(2009)
- J. Sola and A. Gomej-Valent, Int. J. Mod. Phys. D 24, 1541003 ( 2015)
- D. Begue, C. Stahl and S. S. Xue, Nuec. Phys. B 940, 312(2019 )
- G. Risaliti and E. Lusso, Nat. Astron. 3, 272(2019)
- A.G. Riess et al., arXiv:1903.07603[astro-ph.CO]
- S. S. Xue, Nucl. Phys B 897, 326( 2015)
- E.G.M. Ferriera, Phys. Rev. D 95, 043520( 2017)
- T. S. Koivisto, E.N. Saridakis and N. Tamanini, JCAP 1509, 047( 2015)
- S. Kumar and R.C. Nunes, Phys. Rev. D 94, 123511(2016 )
- S. Kumar and R.C. Nunes, Phys. Rev. D 96, 103511( 2017)
- B. Wang, E. Abdulla , F. Atrio-Varandela and D. Pavon, Rept. Prog. Phys 79, 096901(2016).
- L. Amendola, G. Camargo Campos, and R. Rosenfeld, Phys. Rev. D 75, 083506(2007).
- Z. K. Guo, N. Ohta, and S. Tsujikawa, Phys. Rev. D 76, 023508(2007).
- M.S. Berman, II Nuovo Cimento B 74, 1971( 1983).
- M.S. Berman, F.M.Gomide, Gen. Relativ. Gravit. 20, 191(1988).
- A. Pradhan , H. Amirhashchi and B. Saha , Int. J. Theor. Phys. 50, 2923(2011).
- A. Pradhan, Commun. Theor. Phys. 55, 931(2011).
- D.N. Spergel, et al., Astrophys. Jour. Suppl. 170, 377(2007).
- D.Komatsu, et al., Astrophys. Jour. Suppl. Series. 180, 330( 2009).
- T. Padmanabhan, T.R. Choudhury, Mon. Not. R. Astron. Soc. 244, 823(2003).
- L. Amendola, Mon. Not. R. Astron. Soc. 342, 221(2003).
- A. G. Riess, et al., Astrophys. J. Astrophys. 560, 49( 2001).
- Abdusattar and S.R. Prajapati, Astrophys. Space Sci. 335, 657(2011).
- O. Akarsu, et al., Jour. Cosm. Astrop. Phy. 01, 022(2014).
- L. Avile ′ s, et al., Journ. Phys.: Conference series 70 , 012010( 2016).
- S. Kumar, Grav. & Cosm. 19, 284-287(2013).
- A. Pradhan and R. Jaisaval, Int. J. Geom. Methods Mod. Phys. 15, 1850076(2018).
- C.R. Mahanta and N. Sharma, New Astronomy 57, 70(2017).
- A.K. Yadav, et al., Int. J. Theor. Phys. 54, 1671-1679(2015).
- R. Zia, D.C. Maurya and A. Pradhan, Int. J. Geom. Methods Mod. Phys. 15, 1850168(2018).
- A.K. Yadav and V. Bhardwaj, Res. Astron. Astrophys. 18, 64(2016).
- B. Mishra and S.K. Tripathi, Mod. Phys. A 30, 1550175(2015).
- U.K. Sharma, et al., J. Astrophys. Astr. 40, 2(2019).
- P.H.R.S. Moraes, Astrophys. Space Sci. 352, 273-279(2014).
- P.H.R.S. Moraes, G.Ribeiro and R.A.C. Correa, Astrophys. Space Sci. 361, 227( 2016).
- P.H.R.S. Moraes and P.K. Sahoo, Eur. Phys. J. C 77, 480(2017).
- S. Capozziello, et al., Phys. Rev. D 90, 044016( 2014).
- S. Capozziello, et al., Phys. Rev. D 91, 124037( 2015).
- O. Farooq and B.Ratra, Astrophys. J. 766, L7(2013).
- O. Farooq, et al., Astrophys. J. 835, 26 (2017)
- W L Freedman et al, Astrophys. Journ., 553, 47 (2001).
- S H Suyu et al, Astrophys. Jour. 711, 201 (2010).
- N. Jarosik et al, Astrophys. Journ. Suppl. 192, 14 (2010).
- A G Riess et al, Astrophys. Journ., 730, 119 (2011).
- F Beutler et al, Mon. Not. R. Astron. Soc., 416, 3017 (2011).
- S Kumar, Mon. Not. Astron. Soc., 422, 2532 (2012).
- C Zhang et al, Res. Astron. Astrophys., 14, 1 (2014).
- D Stern et al, Jour. Cosmo. Astropart. Phys., 1002, 008 (2010)
- M Moresco, Mon. Not. R. Astron. Soc. 450, L16 (2015).
- J Simon et al, Phys. Rev. D, 71, 123001 (2005).
- N Benitez et al, Astrophys. Jour., 577, L1 (2002).
- M. Turner and A G Riess, Astrophys. Jour., 569, 18 (2002).
- A.R. Liddle and D.H. Lyth Cosmological Inflation and Large-Scale Structure (Cambridge University Press 2000)
- D. M. Scolnic, Astrophys. J. 859, 101(2018).