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C. J. Isham, A. Salam and J. A. Strathdee, “F-dominance of gravity”, Phys. Rev. D 3
1971
Earlier work this paper cites.
D. G. Boulware and S. Deser, “Can gravitation have a finite range?”, Phys. Rev. D 6
1972
Earlier work this paper cites.
D. Comelli, M. Crisostomi, F. Nesti, and L. Pilo, “FRW Cosmology in Ghost Free Massive Gravity from Bigravity”, JHEP 1203
Original
1983
Earlier work this paper cites.
L. H. Ford and T. A. Roman, “Averaged energy conditions and quantum inequalities”, Phys. Rev. D 51
1995
Earlier work this paper cites.
D. Hochberg and M. Visser, “Dynamic wormholes, anti-trapped surfaces, and energy conditions”, Phys. Rev. D 58
1998
Earlier work this paper cites.
L. H. Ford and T. A. Roman, “The Quantum interest conjecture”, Phys. Rev. D 60
1999
Earlier work this paper cites.
C. Barceló and M. Visser, “Twilight for the energy conditions?”, Int. J. Mod. Phys. D 11
2002
Earlier work this paper cites.
R. R. Caldwell, M. Kamionkowski and N. N. Weinberg, “Phantom energy and cosmic doomsday”, Phys. Rev. Lett. 91
2003
Earlier work this paper cites.
C. Cattoën and M. Visser, “Necessary and sufficient conditions for big bangs, bounces, crunches, rips, sudden singularities, and extremality events”, Class. Quant. Grav. 22
2005
Earlier work this paper cites.

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2012

Baccetti, Valentina, Martin-Moruno, Prado, Visser, Matt

We consider the effective stress-energy tensors for the foreground and background sectors in ghost-free bimetric gravity.

By considering the symmetries of the theory, we show that the foreground and background null energy conditions (NECs) are strongly anti-correlated.
In particular, the NECs can only be simultaneously fulfilled when they saturate, corresponding to foreground and background cosmological constants.
In all other situations, either the foreground or the background is subject to a NEC-violating contribution to the total stress-energy.

C. J. Isham, A. Salam and J. A. Strathdee, “F-dominance of gravity”, Phys. Rev. D 3
1971
Earlier work this paper cites.
D. G. Boulware and S. Deser, “Can gravitation have a finite range?”, Phys. Rev. D 6
1972
Earlier work this paper cites.
D. Comelli, M. Crisostomi, F. Nesti, and L. Pilo, “FRW Cosmology in Ghost Free Massive Gravity from Bigravity”, JHEP 1203
Original
1983
Earlier work this paper cites.
L. H. Ford and T. A. Roman, “Averaged energy conditions and quantum inequalities”, Phys. Rev. D 51
1995
Earlier work this paper cites.
D. Hochberg and M. Visser, “Dynamic wormholes, anti-trapped surfaces, and energy conditions”, Phys. Rev. D 58
1998
Earlier work this paper cites.
L. H. Ford and T. A. Roman, “The Quantum interest conjecture”, Phys. Rev. D 60
1999
Earlier work this paper cites.
C. Barceló and M. Visser, “Twilight for the energy conditions?”, Int. J. Mod. Phys. D 11
2002
Earlier work this paper cites.
R. R. Caldwell, M. Kamionkowski and N. N. Weinberg, “Phantom energy and cosmic doomsday”, Phys. Rev. Lett. 91
2003
Earlier work this paper cites.
C. Cattoën and M. Visser, “Necessary and sufficient conditions for big bangs, bounces, crunches, rips, sudden singularities, and extremality events”, Class. Quant. Grav. 22
2005
Earlier work this paper cites.