This analysis explores the new wormhole(WH)solution in the background of teleparallel gravity with minimal matter coupling.To complete this study,we consider the conformal symmetry with non-zero Killing vectors.The ex...This analysis explores the new wormhole(WH)solution in the background of teleparallel gravity with minimal matter coupling.To complete this study,we consider the conformal symmetry with non-zero Killing vectors.The exact shape function is computed by considering the linear equation of state with the phantom regime.The energy conditions are investigated for the calculated shape function with the equation of state parameter.The presence of exotic matter is confirmed due to the violation of the null energy condition.The current study also explores the physical properties of the epicyclic frequencies with quasi-periodic oscillations.In the astrophysical,epicyclic frequencies are extensively employed to explore the self-gravitating system.It is concluded that a stable WH solution is acceptable for WH geometry.展开更多
We study the particle dynamics around a black hole(BH)in f(Q)gravity.First,we investigate the influence of the parameters of f(Q)gravity on the horizon structure of the BH,photon orbits and the radius of the innermost...We study the particle dynamics around a black hole(BH)in f(Q)gravity.First,we investigate the influence of the parameters of f(Q)gravity on the horizon structure of the BH,photon orbits and the radius of the innermost stable circular orbit(ISCO)of massive particles.We further study the effects of the parameters of f(Q)gravity on the shadow cast by the BH.Moreover,we consider weak gravitational lensing using the general method,where we also explore the deflection angle of light rays around the BH in f(Q)gravity in uniform and nonuniform plasma mediums.展开更多
In this manuscript,the traversable wormhole solutions have been explored in modified f(R,G)gravity by taking into consideration the model f(R,G)=R+rG2,where R is the Ricci curvature scalar and G is the Gauss–Bonnet t...In this manuscript,the traversable wormhole solutions have been explored in modified f(R,G)gravity by taking into consideration the model f(R,G)=R+rG2,where R is the Ricci curvature scalar and G is the Gauss–Bonnet term.An acceptable form of the redshift function has been incorporated which is a non-constant in nature along with the implementation of those already defined in literature,the two shape functions namely b(r)=r/exp(r-r0)and b(r)=r0log(r+1)/log(r0+1).It is shown by studying the energy condition and through the graphical analysis that the null energy bounds for the effective energy-momentum tensor are generally violated for the presence of the ordinary matter in modified f(R,G)gravity.Energy conditions associated with the matter content threading the wormhole geometries are evaluated and in general are found to favor the null energy conditions in the vicinity of the wormhole throat,the existence of the nonexotic wormhole geometries threaded by the matter has been confirmed under this gravity.展开更多
基金Grant No.ZC304022919 to support his Postdoctoral Fellowship at Zhejiang Normal University,P.R.China。
文摘This analysis explores the new wormhole(WH)solution in the background of teleparallel gravity with minimal matter coupling.To complete this study,we consider the conformal symmetry with non-zero Killing vectors.The exact shape function is computed by considering the linear equation of state with the phantom regime.The energy conditions are investigated for the calculated shape function with the equation of state parameter.The presence of exotic matter is confirmed due to the violation of the null energy condition.The current study also explores the physical properties of the epicyclic frequencies with quasi-periodic oscillations.In the astrophysical,epicyclic frequencies are extensively employed to explore the self-gravitating system.It is concluded that a stable WH solution is acceptable for WH geometry.
基金funded by the National Natural Science Foundation of China 11975145partly supported by Research Grant FZ-20200929344 and F-FA2021-510 of the Uzbekistan Ministry for Innovative DevelopmentGrant No.ZC304022919 to support his Postdoctoral Fellowship at Zhejiang Normal University
文摘We study the particle dynamics around a black hole(BH)in f(Q)gravity.First,we investigate the influence of the parameters of f(Q)gravity on the horizon structure of the BH,photon orbits and the radius of the innermost stable circular orbit(ISCO)of massive particles.We further study the effects of the parameters of f(Q)gravity on the shadow cast by the BH.Moreover,we consider weak gravitational lensing using the general method,where we also explore the deflection angle of light rays around the BH in f(Q)gravity in uniform and nonuniform plasma mediums.
文摘In this manuscript,the traversable wormhole solutions have been explored in modified f(R,G)gravity by taking into consideration the model f(R,G)=R+rG2,where R is the Ricci curvature scalar and G is the Gauss–Bonnet term.An acceptable form of the redshift function has been incorporated which is a non-constant in nature along with the implementation of those already defined in literature,the two shape functions namely b(r)=r/exp(r-r0)and b(r)=r0log(r+1)/log(r0+1).It is shown by studying the energy condition and through the graphical analysis that the null energy bounds for the effective energy-momentum tensor are generally violated for the presence of the ordinary matter in modified f(R,G)gravity.Energy conditions associated with the matter content threading the wormhole geometries are evaluated and in general are found to favor the null energy conditions in the vicinity of the wormhole throat,the existence of the nonexotic wormhole geometries threaded by the matter has been confirmed under this gravity.
