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In this study, cosmological models are considered, where dark matter and dark energy are coupled and may exchange energy through non-gravitational interactions with one other.
1903
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A.G. Riess, A. V. Filippenko, P. Challis, et al., Observational evidence from supernovae for an accelerating universe and a cosmological constant , Astron. J. , 116
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S. Perlmutter, G. Aldering, G. Goldhaber, et al., Measurements of ω \omega and λ \lambda from 42 highredshift supernovae , Astrophys. J. , 517
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I. Zlatev, L. Wang, and P. J. Steinhardt, Quintessence, cosmic coincidence, and the cosmological constant , Phys. Rev. Lett. , 82
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S. M. Carroll, M. Hoffman, and M. Trodden Can the dark energy equation-of-state parameter ω \omega be less than − 1 -1 ? , Phys. Rev. D , 68
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R.R. Caldwell, M. Kamionkowski, and N. N. Weinberg Phantom energy and cosmic doomsday , Phys. Rev. Lett. , 91
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G.Huey and B.D. Wandelt, Interacting Quintessence, the Coincidence Problem and Cosmic Acceleration , Phys. Rev. D , 74
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2007
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2008
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2008
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2009
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M. P. Hobson, G. P. Efstathiou, and A. N. Lasenby, General Relativity , Cambridge University Press , (2021)
2021
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2021
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2021
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2021
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2009
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2021
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2021
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2021
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2022
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2022
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2022
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2022
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M. A. van der Westhuizen, Dark interactions beyond the Λ \Lambda CDM model , Masters dissertation, North-West University (2022) [ https://repository.nwu.ac.za/handle/10394/39596 ]
2022
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M. A. van der Westhuizen, A. Abebe, Dark coupling: cosmological implications of interacting dark energy and dark matter fluids , SA Inst. Phys. Proceedings, ISBN: 978-0-620-97693-0, SAIP2021 (2022) 386-391 [ http://saip.org.za/Proceedings/Track%20D/63.pdf ]
2022
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