Abstract
Here, we analyse the distribution of self-gravitating collapsing fluid to identify the factors accountable for the energy–density inhomogeneity with the systematic construction in modified Gauss–Bonnet (GB) gravity, by taking the space–time which is spherically symmetric. The modified Einstein’s equations help us to observe the variation in the mass function due to different quantities. The dynamical equations and two differential equations for Weyl curvature are formulated, and used to explore the quantities responsible for the inhomogeneity. Irregularity in the fluid is analysed by taking various cases of fluid, under the effects of \(f\mathcal {(G)}\) theory, where \({\mathcal {G}}\) is a Gauss–Bonnet term.
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T Abbott, F B Abdalla, J Aleksic, S Allam, A Amara, D Bacon, E Balbinot, M Banerji, K Bechtol, A Benoit-Lévy, G M Bernstein, E Bertin, J Blazek, C Bonnett, S Bridle, D Brooks, R J Brunner, E Buckley-Geer, D L Burke, G B Caminha, D Capozzi, J Carlsen, A Carnero-Rosell, M Carollo, M Carrasco-Kind, J Carretero, F J Castander, L Clerkin, T Collett, C Conselice, M Crocce, C E Cunha, C B D’Andrea, L N da Costa, T M Davis, S Desai, H T Diehl, J P Dietrich, S Dodelson, P Doel, A Drlica-Wagner, J Estrada, J Etherington, A E Evrard, J Fabbri, D A Finley, B Flaugher, R J Foley, P Fosalba, J Frieman, J García-Bellido, E Gaztanaga, D W Gerdes, T Giannantonio, D A Goldstein, D Gruen, R A Gruendl, P Guarnieri, G Gutierrez, W Hartley, K Honscheid, B Jain, D J James, T Jeltema, S Jouvel, R Kessler, A King, D Kirk, R Kron, K Kuehn, N Kuropatkin, O Lahav, T S Li, M Lima, H Lin, M A G Maia, M Makler, M Manera, C Maraston, J L Marshall, P Martini, R G McMahon, P Melchior, A Merson, C J Miller, R Miquel, J J Mohr, X Morice-Atkinson, K Naidoo, E Neilsen, R C Nichol, B Nord, R Ogando, F Ostrovski, A Palmese, A Papadopoulos, H V Peiris, J Peoples, W J Percival, A A Plazas, S L Reed, A Refregier, A K Romer, A Roodman, A Ross, E Rozo, E S Rykoff, I Sadeh, M Sako, C Sánchez, E Sanchez, B Santiago, V Scarpine, M Schubnell, I Sevilla-Noarbe, E Sheldon, M Smith, R C Smith, M Soares-Santos, F Sobreira, M Soumagnac, E Suchyta, M Sullivan, M Swanson, G Tarle, J Thaler, D Thomas, R C Thomas, D Tucker, J D Vieira, V Vikram, A R Walker, R H Wechsler, J Weller, W Wester, L Whiteway, H Wilcox, B Yanny, Y Zhang and J Zuntz, Mon. Not. R. Astron. Soc. 460, 1270 (2016)
M J Drinkwater, R J Jurek, C Blake, D Woods, K A Pimbblet, K Glazebrook, R Sharp, M B Pracy, S Brough, M Colless, W J Couch, S M Croom, T M Davis, D Forbes, K Forster, D G Gilbank, M Gladders, B Jelliffe, N Jones, I Li, B Madore, D C Martin, G B Poole, T Small, E Wisnioski, T Wyder and H K C Yee, Mon. Not. R. Astron. Soc. 401, 1429 (2010)
C Blake, S Brough, M Colless, C Contreras, W Couch, S Croom, Croton, T M Davis, M J Drinkwater, K Forster, D Gilbank, M Gladders, K Glazebrook, B Jelliffe, R J Jurek, I Li, B Madore, D C Martin, K Pimbblet, G B Poole, M Pracy, R Sharp, E Wisnioski, D Woods, T K Wyder and H K C Yee, Mon. Not. R. Astron. Soc. 425, 405 (2012)
L Lombriser, Phys. Lett. B 797, 134804 (2019)
Ö Akarsu, N Katırcı and S Kumar, Phys. Rev. D 97, 024011 (2018)
S Capozziello, Int. J. Mod. Phys. D 11, 483 (2002)
T Faulkner, M Tegmark, E F Bunn and Y Mao, Phys. Rev. D 76, 063505 (2007)
T Chiba, Phys. Lett. B 575, 1 (2003)
A L Erickcek, T L Smith and M Kamionkowski, Phys. Rev. D 74, 121501 (2006)
A V Astashenok, S Capozziello and S D Odintsov, J. Cosmol. Astropart. Phys. 2013, 040 (2013)
A V Astashenok, S Capozziello and S D Odintsov, Phys. Rev. D 89, 103509 (2014)
G J Olmo and D R Garcia, Universe 1, 173 (2015)
A Malik, S Ahmad and S Ahmad, New Astron. 79, 101392 (2020)
Z Yousaf, Phys. Scr. 95, 075307 (2020)
S Nojiri and S D Odintsov, Int. J. Geom. Methods Mod. 4, 115 (2007)
T P Sotiriou and V Faraoni, Rev. Mod. Phys. 82, 451 (2010)
S Nojiri and S D Odintsov, Phys. Rep. 505, 59 (2011)
S Capozziello and M De Laurentis, Phys. Rep. 509, 167 (2011)
V Faraoni, S Capozziello, S Capozziello and V Faraoni, Beyond Einstein Gravity 170, 59 (2010)
K Bamba, S Capozziello, S Nojiri and S D Odintsov, Astrophys. Space Sci. 342, 155 (2012)
D Dombriz et al, Entropy 14, 1717 (2012)
A Joyce, B Jain, J Khoury and M Trodden, Phys. Rep. 568, 1 (2015)
K Koyama, Rep. Prog. Phys. 79, 046902 (2016)
K Bamba, S Nojiri and S D Odintsov, arXiv preprint arXiv:1302.4831 (2013)
Z Yousaf, Mod. Phys. Lett. A 34, 1950333 (2019)
K Bamba and S D Odintsov, Symmetry 7, 220 (2015)
S D Odintsov and D Sáez-Gómez, Phys. Lett. B 725, 437 (2013)
K Adhav, Astrophys. Space Sci. 339, 365 (2012)
D R K Reddy, R Santikumar and R L Naidu, Astrophys. Space Sci. 342, 249 (2012)
S Nojiri and S D Odintsov, Phys. Lett. B 631, 1, (2005)
G Cognola, E Elizalde, S Nojiri, S D Odintsov and S Zerbini, Phys. Rev. D 73, 084007 (2006)
S Nojiri, S D Odintsov and O G Gorbunova, J. Phys. A Math. Gen. 39, 6627 (2006)
M Gasperini and G Veneziano, Astropart. Phys. 1, 317 (1993)
A De Felice and S Tsujikawa, Phys. Lett. B 675, 1 (2009)
A De Felice and S Tsujikawa, Phys. Rev. D 80, 063516 (2009)
S Nojiri, S Odintsov and V Oikonomou, Phys. Rep. 692, 1 (2017)
G J Olmo, D Rubiera-Garcia and A Wojnar, Phys. Rep. (2020)
M Z Bhatti, Z Yousaf and A Khadim, Phys. Rev. D 101, 104029 (2020)
I Dwivedi and P Joshi, Class. Quantum Gravity 9, L69 (1992)
J Triginer and D Pavón, Class. Quantum Gravity 12, 689 (1995)
L Herrera, A Di Prisco, J L Hernández-Pastora and N O Santos, Phys. Lett. A 237, 113 (1998)
F C Mena and R Tavakol, Class. Quantum Gravity 16, 435 (1999)
Z Yousaf, K Bamba and M Z Bhatti, Phys. Rev. D 93, 124048 (2016)
Z Yousaf, K Bamba and M Z Bhatti, Phys. Rev. D 95, 024024 (2017)
K Bamba, M Ilyas, M Z Bhatti and Z Yousaf, Gen. Relativ. Gravit. 49, 112 (2017)
M Z Bhatti, Z Yousaf and S Khan, Int. J. Mod. Phys. D 30, 2150097 (2021)
M Z Bhatti and Z Yousaf, Chin. J. Phys. 73, 115 (2021)
M Sharif and Z Yousaf Mon. Not. R. Astron. Soc. 432, 264 (2013)
M Sharif and Z Yousaf Astropart. Phys. 56, 19 (2014)
M Sharif and Z Yousaf, Eur. Phys. J. C 75, 194 (2015), arXiv:1504.04367v1 [gr-qc]
Z Yousaf, M Z Bhatti and H Asad, Phys. Dark Univ. 28, 100527 (2020)
R Goswami, A M Nzioki, S D Maharaj and S G Ghosh, Phys. Rev. D 90, 084011 (2014)
M Sharif and Z Yousaf, Int. J. Theor. Phys. 55, 470 (2016)
R Goswami, A M Nzioki, S D Maharaj and S G Ghosh, Eur. Phys. J. C 77, 1 (2017)
P Kanti, B Kleihaus and J Kunz, Phys. Rev. Lett. 107, 271101 (2011)
P Kanti, R Gannouji and N Dadhich, Phys. Rev. D 92, 041302 (2015)
V K Oikonomou, Phys. Rev. D 92, 124027 (2015)
P Kanti, R Gannouji and N Dadhich, Phys. Rev. D 92, 083524 (2015)
L Herrera, Int. J. Mod. Phys. D 20, 1689 (2011)
M E Cahill and G C McVittie, J. Math. Phys. 11, 1382 (1970)
G F Ellis, Gen. Relativ. Gravit. 41, 581 (2009)
W Stoeger, S Nel, R Maartens and G Ellis, Class. Quantum Gravity 9, 493 (1992)
R Maartens, arXiv preprint arXiv:astro-ph/9609119 (1996)
W Israel and J M Stewart, Ann. Phys. 118, 341 (1979)
G Sposito, V K Gupta and R N Bhattacharya, Adv. Water Resour. 2, 59 (1979)
A Di Prisco, N Falcón, L Herrera, M Esculpi and N Santos, Gen. Relativ. Gravit. 29, 1391 (1997)
Z Yousaf, M Z Bhatti and A Farhat, Ann. Phys. 442, 168935 (2022)
N Banerjee and T Paul, Eur. Phys. J. C 78, 1 (2018)
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Appendix
Appendix
In eq. (15) we have \(\chi _{2}, \chi _3\) and \(\chi _{4}\), which are given as
In eq. (16) we have \(Z_2, Z_3\) and \(Z_4\) whch are given as
\(D_{3}\) in eq. (17) is given by
Values of \(F_{2}, F_{3}\) and \(F_{4}\) in (18) are given as follows:
In eqs (28) and (29) we have \(Z_0\) and \(Z_{1}\), which are written as
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Yousaf, Z., Bhatti, M.Z. & Farhat, A. Causes of energy density inhomogenisation with \(f\mathcal {(G)}\) formalism. Pramana - J Phys 97, 27 (2023). https://doi.org/10.1007/s12043-022-02501-0
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DOI: https://doi.org/10.1007/s12043-022-02501-0