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Implication of Negative Temperature in the Inner Horizon of Reissner-Nordström Black Hole

Journal of Mathematical and Fundamental Sciences · Vol. 49 No. 3 (2017) · hlm. 294–305

DOI
10.5614/j.math.fund.sci.2016.49.3.7
ISSN
2338-5510, 2337-5760
Terbit
2017-12-13
Penerbit
Directorate for Research and Innovation (DRI) ITB
Bahasa
eng

Abstrak

This paper reconsiders the properties of Hawking radiation in the inner horizon of a Reissner-Nordström black hole. Through the correlation between temperature and surface gravity, it is concluded that the temperature of the inner horizon is always negative and that of the outer horizon is always positive. Since negative temperature is hotter than any positive temperature, it is predicted that particle radiation from the inner horizon will move toward the outer horizon. However, unlike temperature, entropy in both horizons remains positive. Following the definition of negative temperature in the inner horizon, it is assured that the entropy of a black hole within a closed system can never decrease. By analyzing the conditions of an extremal black hole, the third law of black hole thermodynamics can be extended to multi-horizon black holes.

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Diana Novita SariAfiliasi tidak diketahui2
Siswoyo SiswoyoAfiliasi tidak diketahui1
Dea AmeliaAfiliasi tidak diketahui1
Anisah Mega AndiniAfiliasi tidak diketahui1
Aisyah Deri Ayu Tungga SafitriAfiliasi tidak diketahui1
Susanti SusantiInstitut Agama Islam Negeri Kendari1
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Sumber metadata: OAI-PMH (metadata jurnal) https://journals.itb.ac.id/index.php/jmfs/oai, pertama di-harvest 9 Nov 2026, terakhir terlihat 9 Nov 2026.
Metadata asli (oai_dc) 
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	<dc:title xml:lang="en-US">Implication of Negative Temperature in the Inner Horizon of Reissner-Nordström Black Hole</dc:title>
	<dc:creator>Tiandho, Yuant</dc:creator>
	<dc:subject xml:lang="en-US">black hole radiation</dc:subject>
	<dc:subject xml:lang="en-US">black hole thermodynamics</dc:subject>
	<dc:subject xml:lang="en-US">entropy</dc:subject>
	<dc:subject xml:lang="en-US">multi-horizon</dc:subject>
	<dc:subject xml:lang="en-US">negative temperature</dc:subject>
	<dc:description xml:lang="en-US">This paper reconsiders the properties of Hawking radiation in the inner horizon of a Reissner-Nordström black hole. Through the correlation between temperature and surface gravity, it is concluded that the temperature of the inner horizon is always negative and that of the outer horizon is always positive. Since negative temperature is hotter than any positive temperature, it is predicted that particle radiation from the inner horizon will move toward the outer horizon. However, unlike temperature, entropy in both horizons remains positive. Following the definition of negative temperature in the inner horizon, it is assured that the entropy of a black hole within a closed system can never decrease. By analyzing the conditions of an extremal black hole, the third law of black hole thermodynamics can be extended to multi-horizon black holes.</dc:description>
	<dc:publisher xml:lang="en-US">Directorate for Research and Innovation (DRI) ITB</dc:publisher>
	<dc:date>2017-12-13</dc:date>
	<dc:type>info:eu-repo/semantics/article</dc:type>
	<dc:type>info:eu-repo/semantics/publishedVersion</dc:type>
	<dc:format>application/pdf</dc:format>
	<dc:identifier>https://journals.itb.ac.id/index.php/jmfs/article/view/2717</dc:identifier>
	<dc:identifier>10.5614/j.math.fund.sci.2016.49.3.7</dc:identifier>
	<dc:source xml:lang="en-US">Journal of Mathematical and Fundamental Sciences; Vol. 49 No. 3 (2017); 294-305</dc:source>
	<dc:source>2338-5510</dc:source>
	<dc:source>2337-5760</dc:source>
	<dc:source>10.5614//j.math.fund.sci.2016.49.3</dc:source>
	<dc:language>eng</dc:language>
	<dc:relation>https://journals.itb.ac.id/index.php/jmfs/article/view/2717/2969</dc:relation>
</oai_dc:dc>