
arXiv: 1803.08815
handle: 11588/717098
Energy conditions can play an important role in defining the cosmological evolution. Specifically acceleration/deceleration of cosmic fluid, as well as the emergence of Big Rip singularities, can be related to the constraints imposed by the energy conditions. Here we discuss this issue for $f(R)$ gravity considering also conformal transformations. Cosmological solutions and equations of state can be classified according to energy conditions. The qualitative change of some energy conditions for transformations from the Jordan frame to the Einstein frame is also observed.
13 pages, to be published in Physics Letters B
General Relativity and Quantum Cosmology; General Relativity and Quantum Cosmology; astro-ph.CO; High Energy Physics - Theory, High Energy Physics - Theory, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Physics, QC1-999, alternative theories of gravity, FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), Relativistic gravitational theories other than Einstein's, including asymmetric field theories, General Relativity and Quantum Cosmology, High Energy Physics - Theory (hep-th), astro-ph.CO, energy conditions, cosmology, Relativistic cosmology, Astrophysics - Cosmology and Nongalactic Astrophysics
General Relativity and Quantum Cosmology; General Relativity and Quantum Cosmology; astro-ph.CO; High Energy Physics - Theory, High Energy Physics - Theory, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Physics, QC1-999, alternative theories of gravity, FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), Relativistic gravitational theories other than Einstein's, including asymmetric field theories, General Relativity and Quantum Cosmology, High Energy Physics - Theory (hep-th), astro-ph.CO, energy conditions, cosmology, Relativistic cosmology, Astrophysics - Cosmology and Nongalactic Astrophysics
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