conformal motion
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2021 ◽  
Vol 1913 (1) ◽  
pp. 012107
Author(s):  
Manjushree Muley ◽  
A R Nagpure ◽  
Prafulla Puri ◽  
Vivek Korde

2020 ◽  
Vol 811 ◽  
pp. 135927 ◽  
Author(s):  
M. Farasat Shamir
Keyword(s):  

2020 ◽  
Vol 35 (29) ◽  
pp. 2050240
Author(s):  
Asifa Ashraf ◽  
G. Mustafa ◽  
Mushtaq Ahmad ◽  
Ibrar Hussain

In this work, the possible existence of wormhole solutions have been investigated in the extended teleparallel [Formula: see text] theory of gravity by incorporating the Lorentzian source of non-commutative geometry through the conformal motion. The physical concept of conformal symmetry becomes more arguable when it is discussed in the background of non-commutative geometry, especially with the Lorentzian source. In this context, two specific different models of the extended teleparallel theory, that is, [Formula: see text], and [Formula: see text] (where [Formula: see text], [Formula: see text], [Formula: see text] being real constants and [Formula: see text] a positive integer) have been studied. The corresponding energy conditions are worked out and are analyzed graphically in the presence of the conformal motion with Lorentzian source. The presence of the exotic matter has been confirmed due to the violation of null energy conditions under some particular conditions, thereby proving the existence of the wormhole geometries in both of the models under investigation. Moreover, the stability of the wormhole geometries via the Tolman-Oppenheimer-Volkov equation has been discussed. It is concluded that these wormhole solutions supported by the non-exotic matter truly exist and are well stable under the extended teleparallel gravity.


2020 ◽  
Vol 418 ◽  
pp. 168184 ◽  
Author(s):  
M. Farasat Shamir ◽  
G. Mustafa
Keyword(s):  

2020 ◽  
Vol 17 (07) ◽  
pp. 2050103
Author(s):  
G. Mustafa ◽  
M. Farasat Shamir ◽  
Asifa Ashraf ◽  
Tie-Cheng Xia

This study explores the wormhole solutions in [Formula: see text] Gravity. For this purpose we assume two sorts of matter density profiles, which satisfy the Gaussian and Lorentzian noncommutative distributions. Further, we employ the conformal motions in the back ground of nonzero conformal killing vectors to find the shape-function from the modified field equations of [Formula: see text] gravity. By defining the connection between Gaussian and Lorentzian noncommutative distributions with conformal Killing vectors, it has been investigated that wormhole solutions would exist under the particular values of involved parameters in [Formula: see text] gravity.


2020 ◽  
Vol 65 ◽  
pp. 163-176 ◽  
Author(s):  
G. Mustafa ◽  
Saira Waheed ◽  
M. Zubair ◽  
Tie-Cheng Xia
Keyword(s):  

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