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Fuzzy black hole models in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mi>f</mml:mi> <mml:mo>(</mml:mo> <mml:mi>G</mml:mi> <mml:mo>)</mml:mo> </mml:math> Gravity

M. YousafDepartment of Mathematics, University of Management and Technology, Johar Town Campus, Lahore-54782, PakistanH. AsadDepartment of Mathematics, University of Management and Technology, Johar Town Campus, Lahore-54782, PakistanBander AlmutairiDepartment of Mathematics, College of Science, King Saud University, P.O.Box 2455 Riyadh 11451, Saudi ArabiaSyed Mustafa HasanDepartment of Mathematics, University of the Punjab, Quaid-i-Azam Campus, Lahore-54590, PakistanMd. Abdullah Saeed KhanInstitute of Advanced Study, Shenzhen University, Shenzhen 518060, Guangdong, People's Republic of China
2024en
ABI

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Abstract In this manuscript, we explore the concept of dark matter black holes, inspired by the Einasto density profile in the background of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:mi>f</mml:mi> <mml:mo stretchy="false">(</mml:mo> <mml:mi class="MJX-tex-calligraphic" mathvariant="script">G</mml:mi> <mml:mo stretchy="false">)</mml:mo> </mml:math> gravity, where <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:mi class="MJX-tex-calligraphic" mathvariant="script">G</mml:mi> </mml:math> is a Gauss-Bonnet invariant. This work extends the scope beyond the noncommutative tiny black hole structure which incorporates dark matter as a constituent forming the black hole. Our investigation demonstrates the feasibility of constructing black hole solutions for various Einasto index values, <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:mi>f</mml:mi> <mml:mo stretchy="false">(</mml:mo> <mml:mi class="MJX-tex-calligraphic" mathvariant="script">G</mml:mi> <mml:mo stretchy="false">)</mml:mo> </mml:math> gravity parameters, and parameters of mass function adopting anisotropic fluid configuration to characterize the matter sector. Specifically, by adopting an equation of state in which the radial pressure equals the negative of the energy density, we derive black hole solutions exhibiting a horizon structure with the central singularity replaced by a regular de Sitter core akin to the Reissner-Nordström black holes. Furthermore, we explore an alternative scenario where the equation of state is nonlocal, resulting in the construction of self-gravitating fuzzy dark matter droplets together with the dark source <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:mi>f</mml:mi> <mml:mo stretchy="false">(</mml:mo> <mml:mi class="MJX-tex-calligraphic" mathvariant="script">G</mml:mi> <mml:mo stretchy="false">)</mml:mo> </mml:math> corrections.

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