Abstract
Considering a homogeneous and isotropic Universe characterised by the Friedmann–Lemaître–Robertson–Walker line element, in this work, we have prescribed a general formalism for the cosmological solutions when the equation of state of the cosmic substance follows the general structure \(\phi (p, \rho ) = 0\), where \(p,\,\rho \) are respectively the pressure and the energy density of the cosmic substance. Using the general formalism we recover some well-known solutions, namely, when the cosmic substance obeys the linear equation of state, a Chaplygin-type equation of state, or a nonlinear equation of state. Thus, the current work offers a new technique to solve the cosmological solutions without any prior relation between p and \(\rho \).
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Acknowledgements
SP acknowledges Science and Engineering Research Board (SERB), Govt. of India for National Post-Doctoral Fellowship (File No. PDF / 2015 / 000640). Also, SP thanks the Department of Mathematics, Jadavpur University where a part of the work was carried out.
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Das, A., Banerjee, A., Chakraborty, S. et al. Perfect fluid cosmological Universes: One equation of state and the most general solution. Pramana - J Phys 90, 19 (2018). https://doi.org/10.1007/s12043-017-1511-z
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DOI: https://doi.org/10.1007/s12043-017-1511-z