# Hawking Radiation Of Regular Hayward Black Hole Surrounded By Quintessence

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### Accretion and evaporation of modiﬁed Hayward black hole

mass of the black hole during accretion of the ﬂuid ﬂow, taking into consideration Hawking radiation from the black hole, i.e., evaporation of the black hole, is analyzed. 1 Introduction At present we live in a Universe which is expanding and the expansion rate is increasing, i.e., the Universe is accel-

### A note on temperature and energy of four-dimensional black

29/8/2020 Quantum Gravity Correction to Hawking Radiation of the 2+1-Dimensional Wormhole Ganim Gecim and Yusuf Sucu-Thermodynamic phase transition and global stability of the regular Hayward black hole surrounded by quintessence Kamiko Kouemeni Jean Rodrigue et al-Thermodynamics and Phase Transition from Regular Bardeen Black Hole Surrounded by Quintessence

### Surrounded Vaidya solution by cosmological fields

physical explanation for a black hole mass diminishing may be is that accreting particles of a phantom scalar ﬁeld have a total negative energy [103]. Similar particles possessing negative energies are created through the Hawking radiation processandalsointheenergyextractionprocessfromablack hole by the Penrose mechanism. The effect of phantom-like dark energy onto a charged Reissner Nordström black hole

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7/6/2019 Hawking radiation of the same temperature. This can be achieved trivially by having the black-hole horizon coincide with the de Sitter horizon, but we can also have a more interesting situation where the horizons are separate. The gravitational instantons

### arXiv:2008.00061v3 [gr-qc] 6 Nov 2020

using the metric of the black hole surrounded by quintessence and the deﬁnition of the eﬀective potential, we analyzed in detail the null geodesics for diﬀerent energies. We also described the horizons of the Hayward black hole surrounded by quintessence as well as the shadow of the black hole. PACS numbers: 04.20.-q, 04.70.-s, 04.70.Bw, 04.20.Dw

### arXiv:1808.03474v2 [gr-qc] 27 Jul 2020

for the regular Hayward black hole surrounded by quintessence is T = mr(r3 −4β2) 2π(r3 +2β2)2 + (3ωq +1)a 4πr(3ωq +2). (10) Considering only the quantum eﬀects (β 6= 0 and a = 0), this expression of the Unruh-Verlinde temperature is reduced to T = (). = +. =,