On the existence and stability of traversable wormhole solutions with novel shapefunctions in the framework of F(R,L_(m))gravity

作     者：Sourav Chaudhary Jitendra Kumar S K Maurya Sweeti Kiroriwal Abdul Aziz Sourav Chaudhary;Jitendra Kumar;S K Maurya;Sweeti Kiroriwal;Abdul Aziz

作者机构：Department of MathematicsCentral University of HaryanaJant-PaliMahendergarhIndia Department of Mathematical and Physical SciencesCollege of Arts and ScienceUniversity of NizwaP.O.Box 33Nizwa 616Oman 

出 版 物：《Communications in Theoretical Physics》 (理论物理通讯（英文版）)

年 卷 期：2024年第76卷第5期

页      面：114-127页

核心收录：

学科分类：07[理学] 070201[理学-理论物理] 0702[理学-物理学] 

基　　金：S Chaudhary expresses his gratitude to the Central University of Haryana for providing a University Research Fellowship (URF) under the Reg. No. 222019 the Department of Mathematics, Central University of Haryana the University Grant Commission (UGC), New Delhi, India under the NTA Ref. No. 211610000030 for providing financial support 

主　　题：energy conditions wormhole exotic matter F(R L_(m))gravity 

摘      要：In this work,we have explored wormhole(WH)solutions in F(R,L_(m))gravity by assuming the Morris-Thorne WH metric and F(R,Lm)=R/2+(1+γR)L_(m),whereγis the free model *** determined the WH solutions by utilizing two newly developed shape functions(SF)that satisfy all basic conditions for a WH’s physical *** also observe that the null energy condition(NEC)behaves ***,for both models,we use the volume integral quantifier(VIQ)and Tolman-Oppenheimer-Volkoff(TOV)equation to determine how much exotic matter is needed near the WH throat and the stability of the *** extensive detailed discussions of the matter components have been done via graphical *** obtained WH geometries meet the physically acceptable conditions for a stable wormhole.