2020
DOI: 10.1103/physrevd.102.084027
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Black holes in torsion bigravity

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Cited by 8 publications
(5 citation statements)
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“…where R αµβν is the background Riemann tensor, is allowed in a Ricci-flat background, thus modifying the Fierz-Pauli mass term. Notice that this term is absent from the bimetric expansion around Minkowski (2.11), but, as highlighted in [47], may appear in ghost-free and tachyon-free torsion bigravity [48][49][50][51][52][53]. The latter is a type of generalized Einstein-Cartan theory with propagating torsion and importantly has a subclass with the same spectrum as ghost-free bimetric theory around Minkowski spacetime [54][55][56][57].…”
Section: Expanding Around Equal Backgroundsmentioning
confidence: 96%
“…where R αµβν is the background Riemann tensor, is allowed in a Ricci-flat background, thus modifying the Fierz-Pauli mass term. Notice that this term is absent from the bimetric expansion around Minkowski (2.11), but, as highlighted in [47], may appear in ghost-free and tachyon-free torsion bigravity [48][49][50][51][52][53]. The latter is a type of generalized Einstein-Cartan theory with propagating torsion and importantly has a subclass with the same spectrum as ghost-free bimetric theory around Minkowski spacetime [54][55][56][57].…”
Section: Expanding Around Equal Backgroundsmentioning
confidence: 96%
“…where R αµβν is the background Riemann tensor, is allowed in a Ricci-flat background, thus modifying the Fierz-Pauli mass term. Notice that this term is absent from the bimetric expansion around Minkowski (2.11), but, as highlighted in [60], may appear in ghost-free and tachyon-free torsion bigravity [61][62][63][64][65][66]. The latter is a type of generalized Einstein-Cartan theory with propagating torsion and importantly has a subclass with the same spectrum as ghost-free bimetric theory around Minkowski spacetime [67][68][69][70].…”
Section: Jhep12(2021)220mentioning
confidence: 96%
“…Various aspects of exact or numerical solutions of the class II torsion gravity field equations it provides have been discussed in the litterature (see for instance refs. [18,19,22,27,28]). Here after we shall display some exact solutions of models of classes I and II, mainly in order to illustrate the differences between the two.…”
Section: Special Solutionsmentioning
confidence: 99%
“…. [27,28]. They rest on a static spherically symmetric geometry written in Schwarzschild coordinates :…”
Section: A Black-hole Solutionmentioning
confidence: 99%