The method of minimal geometric deformation (MGD) is used to derive static, strongly gravitating, spherically symmetric, compact stellar distributions. The trace and Weyl anomalies are then employed to probe the MGD in the holographic setup, as a realistic model, playing a prominent role in AdS/CFT. (C) 2021 The Author(s). Published by Elsevier B.V.
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Chulalongkorn Univ, Fac Sci, Dept Phys, High Energy Phys Theory Grp, Bangkok 10330, ThailandChulalongkorn Univ, Fac Sci, Dept Phys, High Energy Phys Theory Grp, Bangkok 10330, Thailand
Burikham, Piyabut
Harko, Tiberiu
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Natl Inst Phys & Nucl Engn IFIN HH, Dept Theoret Phys, Bucharest 077125, Romania
Babes Bolyai Univ, Dept Phys, Kogalniceanu St, Cluj Napoca 400084, Romania
Astron Observ, 19 Ciresilor St, Cluj Napoca 400487, RomaniaChulalongkorn Univ, Fac Sci, Dept Phys, High Energy Phys Theory Grp, Bangkok 10330, Thailand
Harko, Tiberiu
Pimsamarn, Kulapant
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Kasetsart Univ, Fac Sci, Dept Phys, Bangkok 10900, ThailandChulalongkorn Univ, Fac Sci, Dept Phys, High Energy Phys Theory Grp, Bangkok 10330, Thailand
Pimsamarn, Kulapant
Shahidi, Shahab
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Damghan Univ, Sch Phys, Damghan 4116736716, IranChulalongkorn Univ, Fac Sci, Dept Phys, High Energy Phys Theory Grp, Bangkok 10330, Thailand