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• W4308657619 abstract "This work aims to study the accretions of dark energy coupled with dark matter onto a static Schwarzschild black hole of [Formula: see text] dimensions. Besides the accretion of fluids, the effect due to evaporation of black hole of [Formula: see text] dimensions is under consideration. Mass is one of the interesting dynamical properties of a black hole. The changes in masses have been projected in the framework of the Friedmann–Robertson–Walker model of the universe of [Formula: see text] dimensions. The [Formula: see text]-type Pilgrim dark energies with their logarithmic and power-law entropy corrections are considered as the form of dark energy in our study. Further, the scale factor that is considered as [Formula: see text], [Formula: see text] follows the power-law form. The changes in the dynamical mass of the black hole have been calculated with the variation corresponding to redshift [Formula: see text] while dark matter and specified type of dark energy accrete onto [Formula: see text]-dimensional Schwarzschild black hole. It is found that the dynamical mass of the black hole increases in the late-time epoch as a consequence of the prescribed form of dark energy accretion and evaporation of the black hole. Finally, we discuss the accretion phenomena of the above-specified types of dark energies onto [Formula: see text]-dimensional Morris–Thorne wormhole. It has been investigated that the masses of the black hole and the wormhole sensitively vary with the values of the dimensions." @default.
• W4308657619 created "2022-11-13" @default.
• W4308657619 creator A5021728811 @default.
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• W4308657619 date "2022-08-30" @default.
• W4308657619 modified "2023-09-26" @default.
• W4308657619 title "Accretions of (<i>m</i>, <i>n</i>)-type Pilgrim dark energies with logarithmic and power-law entropy corrections onto (<i>D</i> + <i>2</i>)-dimensional black hole and wormhole" @default.
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• W4308657619 doi "https://doi.org/10.1142/s0217732322501735" @default.
• W4308657619 hasPublicationYear "2022" @default.
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