Reconstructing wormhole solutions in curvature based Extended Theories of Gravity

Abstract Static and spherically symmetric wormhole solutions can be reconstructed in the framework of curvature based Extended Theories of Gravity. In particular, extensions of the General Relativity, in metric and curvature formalism give rise to modified gravitational potentials, constituted by th...

Full description

Bibliographic Details
Main Authors: Vittorio De Falco, Emmanuele Battista, Salvatore Capozziello, Mariafelicia De Laurentis
Format: Article
Language:English
Published: SpringerOpen 2021-02-01
Series:European Physical Journal C: Particles and Fields
Online Access:https://doi.org/10.1140/epjc/s10052-021-08958-4
id doaj-d24ea02668cb4a25ae8d075cf57dd2d6
record_format Article
spelling doaj-d24ea02668cb4a25ae8d075cf57dd2d62021-02-21T12:43:37ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522021-02-018121910.1140/epjc/s10052-021-08958-4Reconstructing wormhole solutions in curvature based Extended Theories of GravityVittorio De Falco0Emmanuele Battista1Salvatore Capozziello2Mariafelicia De Laurentis3Department of Mathematics and Applications “R. Caccioppoli”, University of Naples Federico IIInstitute for Theoretical Physics, Karlsruhe Institute of Technology (KIT)Università degli studi di Napoli “Federico II”, Dipartimento di Fisica “Ettore Pancini”, Complesso Universitario di Monte S. AngeloUniversità degli studi di Napoli “Federico II”, Dipartimento di Fisica “Ettore Pancini”, Complesso Universitario di Monte S. AngeloAbstract Static and spherically symmetric wormhole solutions can be reconstructed in the framework of curvature based Extended Theories of Gravity. In particular, extensions of the General Relativity, in metric and curvature formalism give rise to modified gravitational potentials, constituted by the classical Newtonian potential and Yukawa-like corrections, whose parameters can be, in turn, gauged by the observations. Such an approach allows to reconstruct the spacetime out of the wormhole throat considering the asymptotic flatness as a physical property for the related gravitational field. Such an argument can be applied for a large class of curvature theories characterising the wormholes through the parameters of the potentials. According to this procedure, possible wormhole solutions could be observationally constrained. On the other hand, stable and traversable wormholes could be a direct probe for this class of Extended Theories of Gravity.https://doi.org/10.1140/epjc/s10052-021-08958-4
collection DOAJ
language English
format Article
sources DOAJ
author Vittorio De Falco
Emmanuele Battista
Salvatore Capozziello
Mariafelicia De Laurentis
spellingShingle Vittorio De Falco
Emmanuele Battista
Salvatore Capozziello
Mariafelicia De Laurentis
Reconstructing wormhole solutions in curvature based Extended Theories of Gravity
European Physical Journal C: Particles and Fields
author_facet Vittorio De Falco
Emmanuele Battista
Salvatore Capozziello
Mariafelicia De Laurentis
author_sort Vittorio De Falco
title Reconstructing wormhole solutions in curvature based Extended Theories of Gravity
title_short Reconstructing wormhole solutions in curvature based Extended Theories of Gravity
title_full Reconstructing wormhole solutions in curvature based Extended Theories of Gravity
title_fullStr Reconstructing wormhole solutions in curvature based Extended Theories of Gravity
title_full_unstemmed Reconstructing wormhole solutions in curvature based Extended Theories of Gravity
title_sort reconstructing wormhole solutions in curvature based extended theories of gravity
publisher SpringerOpen
series European Physical Journal C: Particles and Fields
issn 1434-6044
1434-6052
publishDate 2021-02-01
description Abstract Static and spherically symmetric wormhole solutions can be reconstructed in the framework of curvature based Extended Theories of Gravity. In particular, extensions of the General Relativity, in metric and curvature formalism give rise to modified gravitational potentials, constituted by the classical Newtonian potential and Yukawa-like corrections, whose parameters can be, in turn, gauged by the observations. Such an approach allows to reconstruct the spacetime out of the wormhole throat considering the asymptotic flatness as a physical property for the related gravitational field. Such an argument can be applied for a large class of curvature theories characterising the wormholes through the parameters of the potentials. According to this procedure, possible wormhole solutions could be observationally constrained. On the other hand, stable and traversable wormholes could be a direct probe for this class of Extended Theories of Gravity.
url https://doi.org/10.1140/epjc/s10052-021-08958-4
work_keys_str_mv AT vittoriodefalco reconstructingwormholesolutionsincurvaturebasedextendedtheoriesofgravity
AT emmanuelebattista reconstructingwormholesolutionsincurvaturebasedextendedtheoriesofgravity
AT salvatorecapozziello reconstructingwormholesolutionsincurvaturebasedextendedtheoriesofgravity
AT mariafeliciadelaurentis reconstructingwormholesolutionsincurvaturebasedextendedtheoriesofgravity
_version_ 1724257855039602688