HAWKING TEMPERATURE IN SCHWARZSCHILD BLACK HOLES WITH QUINTESSENCE DARK ENERGY

Agustina Widiyani; Ana Novita  Sari; Ikah Ning Prasetiowati  Permanasari; Eko  Satria; Azrul Sulaiman Karim  Pohan; Weni Ayu Puja  Kesuma; Indra  Pardede; Agus  Suroso

doi:10.29303/ipr.v8i2.454

HAWKING TEMPERATURE IN SCHWARZSCHILD BLACK HOLES WITH QUINTESSENCE DARK ENERGY

Authors

Agustina Widiyani , Ana Novita Sari , Ikah Ning Prasetiowati Permanasari , Eko Satria , Azrul Sulaiman Karim Pohan , Weni Ayu Puja Kesuma , Indra Pardede , Agus Suroso

DOI:

10.29303/ipr.v8i2.454

Published:

2025-05-25

Issue:

Vol. 8 No. 2 (2025)

Keywords:

Hawking temperature, Black hole, Schwarzschild de-Sitter, quintessence

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Widiyani, A., Sari, A. N. ., Permanasari, I. N. P. ., Satria, E. ., Pohan, A. S. K. ., Kesuma, W. A. P. ., Pardede, I., & Suroso, A. . (2025). HAWKING TEMPERATURE IN SCHWARZSCHILD BLACK HOLES WITH QUINTESSENCE DARK ENERGY. Indonesian Physical Review, 8(2), 553–568. https://doi.org/10.29303/ipr.v8i2.454

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Abstract

Black holes are thermodynamic objects that emit Hawking radiation near the event horizon of a black hole according to the theory of quantum gravity in curved space-time. This radiation is manifested as the temperature of a black hole, known as the Hawking temperature. According to black hole thermodynamics, the black hole horizon area corresponds to the entropy. The increase in the horizon area is predicted due to the influence of dark energy, which can push the horizon of the black hole away from its center, thus significantly affecting the radiation of the black hole. Here, we investigate the Hawking temperature of the Schwarzschild black hole under the effect of quintessence dark energy. The results show that the increase in quintessence reduces the horizon radius of the black hole and lowers its Hawking temperature, highlighting the direct relationship between dark energy and black hole dynamics.

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HAWKING TEMPERATURE IN SCHWARZSCHILD BLACK HOLES WITH QUINTESSENCE DARK ENERGY

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