2021
DOI: 10.3390/sym14010032
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Uniqueness of the Inflationary Higgs Scalar for Neutron Stars and Failure of Non-Inflationary Approximations

Abstract: Neutron stars are perfect candidates to investigate the effects of a modified gravity theory, since the curvature effects are significant and more importantly, potentially testable. In most cases studied in the literature in the context of massive scalar-tensor theories, inflationary models were examined. The most important of scalar-tensor models is the Higgs model, which, depending on the values of the scalar field, can be approximated by different scalar potentials, one of which is the inflationary. Since i… Show more

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Cited by 13 publications
(1 citation statement)
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“…One way of modifying gravity consists of replacing the original Einstein-Hilbert Lagrangian by an arbitrary function of its original argument, as has been done, for instance, in f (R) theories [18][19][20][21][22][23][24][25][26][27]. An example is Starobinsky's model, where he proposed a modification of the Einstein-Hilbert action by including a square term R 2 , which could explain the early inflation of the universe [28][29][30][31]. As can be verified in several works, these modified theories are usually good candidates to replace the dark energy sector [15,16].…”
Section: Introductionmentioning
confidence: 99%
“…One way of modifying gravity consists of replacing the original Einstein-Hilbert Lagrangian by an arbitrary function of its original argument, as has been done, for instance, in f (R) theories [18][19][20][21][22][23][24][25][26][27]. An example is Starobinsky's model, where he proposed a modification of the Einstein-Hilbert action by including a square term R 2 , which could explain the early inflation of the universe [28][29][30][31]. As can be verified in several works, these modified theories are usually good candidates to replace the dark energy sector [15,16].…”
Section: Introductionmentioning
confidence: 99%