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Journal articles on the topic 'Black holes'

Author: Grafiati

Published: 4 June 2021

Last updated: 25 July 2025

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1

Krauss, Lawrence M., Hong Liu, and Junseong Heo. "Dirty Black Holes and Hairy Black Holes." Physical Review Letters 77, no. 26 (1996): 5164–67. http://dx.doi.org/10.1103/physrevlett.77.5164.

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2

WALD, R. "The Physics of Black Holes: Black Holes." Science 234, no. 4778 (1986): 882. http://dx.doi.org/10.1126/science.234.4778.882.

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3

Rovelli, Carlo. "Black holes." Europhysics News 52, no. 1 (2021): 16–18. http://dx.doi.org/10.1051/epn/2021102.

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They are out there in the sky in huge numbers. They are the most astonishing objects in the universe. Their existence was predicted and understood before we detected them. They behave precisely as the theory predicted. Yet, we do not know what happens at their center, nor in their future. But this confusion is our key towards what we most lack in fundamental physics: understanding quantum gravity.

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4

Capossere, Bill. "Black Holes." Colorado Review 36, no. 1 (2009): 129–43. http://dx.doi.org/10.1353/col.2009.0051.

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5

Šimečka, Milan. "Black holes." Index on Censorship 17, no. 5 (1988): 52–56. http://dx.doi.org/10.1080/03064228808534431.

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6

Novikov*, I. D. "Black holes." Surveys in High Energy Physics 18, no. 1-4 (2003): 139–54. http://dx.doi.org/10.1080/01422410310001610464.

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7

Horowitz, Gary T., and Saul A. Teukolsky. "Black holes." Reviews of Modern Physics 71, no. 2 (1999): S180—S186. http://dx.doi.org/10.1103/revmodphys.71.s180.

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8

Brugmann, B., A. M. Ghez, and J. Greiner. "Black holes." Proceedings of the National Academy of Sciences 98, no. 19 (2001): 10525–26. http://dx.doi.org/10.1073/pnas.201365798.

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9

Ferreira, Pedro. "Black holes." New Scientist 207, no. 2767 (2010): iv. http://dx.doi.org/10.1016/s0262-4079(10)61577-1.

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10

Jamshid, Mossayeb. "Black holes." Astronomy Quarterly 7, no. 1 (1990): 35–49. http://dx.doi.org/10.1016/0364-9229(90)90010-x.

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11

Creighton, Teviet, and Richard Price. "Black holes." Scholarpedia 3, no. 1 (2008): 4277. http://dx.doi.org/10.4249/scholarpedia.4277.

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12

Karouzos, Marios. "Black holes." Nature Astronomy 3, no. 1 (2019): 2–5. http://dx.doi.org/10.1038/s41550-018-0671-1.

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13

Gunn, Angel Sands. "Black Holes." Appalachian Heritage 42, no. 4 (2014): 77–91. http://dx.doi.org/10.1353/aph.2014.0087.

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14

Bisnovatyi-Kogan, G. S. "Black Holes." Astronomy Reports 68, S1 (2024): S10—S13. https://doi.org/10.1134/s1063772924701087.

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15

Zaslavskii, O. B. "Truly naked black holes and quasi-black holes." Gravitation and Cosmology 14, no. 1 (2008): 60–64. http://dx.doi.org/10.1134/s0202289308010088.

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16

Lifschytz, Gilad. "Charged black holes from near extremal black holes." Journal of High Energy Physics 2004, no. 09 (2004): 009. http://dx.doi.org/10.1088/1126-6708/2004/09/009.

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17

Grib, A. A. "Are black holes black?" Soviet Physics Journal 32, no. 5 (1989): 401–3. http://dx.doi.org/10.1007/bf00895326.

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18

Haldar, Amritendu, and Ritabrata Biswas. "Thermodynamic studies of different type of black holes: General uncertainty principle approach." Modern Physics Letters A 33, no. 34 (2018): 1850200. http://dx.doi.org/10.1142/s0217732318502000.

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We present an investigation on thermodynamics of two different types of black holes viz. Kiselev black hole (asymptotically flat) and Taub–NUT (non-asymptotically flat) black hole. We compute the thermodynamic variables like black hole’s Hawking temperature and entropy at the black hole’s event horizon. Further, we derive the heat capacity and examine it to study the thermal stability of the black holes. We also calculate the rate of emission, assuming the black holes radiate energy in terms of photons by tunneling. We graphically represent all the parameters including the rate of emission of

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19

Joo, Denes. "Black Holes – Wormholes – White Holes." Open Access Journal of Chemistry 7, no. 1 (2025): 45–60. https://doi.org/10.22259/2637-5834.0701003.

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20

Sammy, Kumari, and Sumita Singh. "Homoclinic Orbit of Kerr Black Holes." Indian Journal Of Science And Technology 17, no. 44 (2024): 4582–88. https://doi.org/10.17485/ijst/v17i44.3029.

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Objective: This study investigates the effective potential and homoclinic orbit near the Kerr metric system of black holes. It also examines the graphical relationship between effective potential and radial momentum with distance from black holes. Methods: The motion of a test particle near the Kerr metric has been analyzed using the Euler Lagrangian and action-angle variable methods. The graphical analysis in this study was performed with Mathematica software. Findings: An expression for effective potential and radial momentum has been evaluated. It has been shown that homoclinic orbits exist

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21

Fishbach, Maya, Daniel E. Holz, and Ben Farr. "Are LIGO's Black Holes Made from Smaller Black Holes?" Astrophysical Journal 840, no. 2 (2017): L24. http://dx.doi.org/10.3847/2041-8213/aa7045.

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22

Li, Miao. "Macroscopic black holes, microscopic black holes and noncommutative membrane." Classical and Quantum Gravity 21, no. 14 (2004): 3571–78. http://dx.doi.org/10.1088/0264-9381/21/14/016.

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23

Unruh, W. G. "Dumb holes: analogues for black holes." Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 366, no. 1877 (2008): 2905–13. http://dx.doi.org/10.1098/rsta.2008.0062.

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The use of sonic analogues to black and white holes, called dumb or deaf holes, to understand the particle production by black holes is reviewed. The results suggest that the black hole particle production is a low-frequency and low-wavenumber process.

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24

Courvoisier, T. J. L., and B. Wilkes. "High-Energy Radiation from Black Holes: From Supermassive Black Holes to Galactic Solar Mass Black Holes." Advances in Space Research 38, no. 7 (2006): 1345. http://dx.doi.org/10.1016/j.asr.2006.06.001.

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25

Grib, A. A., and Yu V. Pavlov. "Are black holes totally black?" Gravitation and Cosmology 21, no. 1 (2015): 13–18. http://dx.doi.org/10.1134/s0202289315010065.

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26

Genzel, Reinhard. "How black holes stay black." Nature 391, no. 6662 (1998): 17–18. http://dx.doi.org/10.1038/34029.

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27

Lee, T. D. "Are black holes black bodies?" Nuclear Physics B 264 (January 1986): 437–86. http://dx.doi.org/10.1016/0550-3213(86)90493-1.

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28

Mu, Benrong, Peng Wang, and Haitang Yang. "Minimal Length Effects on Tunnelling from Spherically Symmetric Black Holes." Advances in High Energy Physics 2015 (2015): 1–8. http://dx.doi.org/10.1155/2015/898916.

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We investigate effects of the minimal length on quantum tunnelling from spherically symmetric black holes using the Hamilton-Jacobi method incorporating the minimal length. We first derive the deformed Hamilton-Jacobi equations for scalars and fermions, both of which have the same expressions. The minimal length correction to the Hawking temperature is found to depend on the black hole’s mass and the mass and angular momentum of emitted particles. Finally, we calculate a Schwarzschild black hole's luminosity and find the black hole evaporates to zero mass in infinite time.

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29

Luc Wendkouni TOUGMA, Jean, Sie Zacharie KAM, and Jean KOULIDIATI. "Quantum Information Reaching the Black Holes." International Journal of Science and Research (IJSR) 10, no. 12 (2021): 1181–91. https://doi.org/10.21275/mr211224033254.

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30

Hsu, Stephen D. H. "White holes and eternal black holes." Classical and Quantum Gravity 29, no. 1 (2011): 015004. http://dx.doi.org/10.1088/0264-9381/29/1/015004.

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31

Düztaş, Koray, and Mubasher Jamil. "String analog of Reissner–Nordström black holes cannot be overcharged." Modern Physics Letters A 34, no. 30 (2019): 1950248. http://dx.doi.org/10.1142/s0217732319502481.

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In this work, we attempt to overcharge extremal and nearly extremal charged black holes in string theory, known as the Garfinkle–Horowitz–Strominger solution. We first show that extremal black holes cannot be overcharged analogous to the case of Reissner–Nordström (RN) black holes. Contrary to their analog in general relativity, nearly extremal black holes can neither be overcharged beyond extremality, nor can they be driven to extremality by the interaction with test particles. Therefore, the analysis in this work also implies that the third law of black hole thermodynamics holds for the rele

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32

Palchoudhury, Sankar. "About Black Holes." International Journal of Fundamental Physical Sciences 11, no. 1 (2021): 6–9. http://dx.doi.org/10.14331/ijfps.2021.330144.

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All kinds of waves occur for the disturbances in the quiet gravitational field. Different waves powered differently and propagated in the gravitational field. A black hole is the higher GFI (Gravitational Field Intensity) area. The rays do not possess, coming from a distant source when pass by the black holes, adequate strength to disturb in the higher GFI area of the black holes. Naturally, the rays take on a curve path as the provision in a circular area depends on the radius (distance), keeping distance according to the lower GFI area around the black holes’ centre.

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33

Steiner, George. "Some Black Holes." Bulletin of the American Academy of Arts and Sciences 41, no. 2 (1987): 12. http://dx.doi.org/10.2307/3822663.

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34

Aliev, A. N., and D. V. Gal'tsov. ""Magnetized" black holes." Uspekhi Fizicheskih Nauk 157, no. 1 (1989): 129. http://dx.doi.org/10.3367/ufnr.0157.198901d.0129.

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35

Dalton, Kenneth. "Supermassive Black Holes." Journal of High Energy Physics, Gravitation and Cosmology 05, no. 03 (2019): 984–88. http://dx.doi.org/10.4236/jhepgc.2019.53052.

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36

de Valk, Giliam. "Analytic Black Holes." National security and the future 23, no. 1 (2022): 21–48. http://dx.doi.org/10.37458/nstf.23.1.1.

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In Analytic Black Holes it is advocated to start a new, second, revolution in security and intelligence analysis. After the first revolution, which started in the Netherlands as late as 2006 with the massive training in Structured Analytic Techniques at both the academia and at the MoD (e.g. Defense Intelligence and Security Institute). A new second revolution – that of Augmented Intelligence – is at hand as a result of two developments, the change in data flows and the need for new products. Data are exploding, especially unstructured data. But the majority of the data remains unused in analy

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37

Shurcliff, William A. "Black Holes—"Ingestars"?" Science 231, no. 4744 (1986): 1355. http://dx.doi.org/10.1126/science.231.4744.1355.f.

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38

Bizon, Piotr. "Colored black holes." Physical Review Letters 64, no. 24 (1990): 2844–47. http://dx.doi.org/10.1103/physrevlett.64.2844.

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39

de Freitas Pacheco, José Antonio. "Dormant Black Holes." International Journal of Modern Physics: Conference Series 45 (January 2017): 1760022. http://dx.doi.org/10.1142/s2010194517600229.

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The growth of supermassive black holes is intermittent, having periods of low accretion when no nuclear activity is seen in the center of the host galaxy. In such dormant state black holes may tidally disrupt stars scattered from the bulge to inside their influence sphere. The resulting debris are partially captured by the black hole forming a short-lived accretion disk, which produces a variable emission dubbed “tidal flare”. Some galaxies candidate to have hosted these tidal events are here considered.

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40

Ho, Pei-Ming. "Asymptotic black holes." Classical and Quantum Gravity 34, no. 8 (2017): 085006. http://dx.doi.org/10.1088/1361-6382/aa641e.

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41

Derbes, David. "Exploring Black Holes." American Journal of Physics 89, no. 1 (2021): 121–23. http://dx.doi.org/10.1119/10.0002493.

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42

Buchanan, Mark. "Defining black holes." Nature Physics 14, no. 10 (2018): 970. http://dx.doi.org/10.1038/s41567-018-0299-1.

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43

Zeng, Xiaoxiong, Christian Corda, and Deyou Chen. "Black Holes Physics." Advances in High Energy Physics 2014 (2014): 1–2. http://dx.doi.org/10.1155/2014/453586.

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44

Lasota, Jean-Pierre. "Unmasking Black Holes." Scientific American 280, no. 5 (1999): 40–47. http://dx.doi.org/10.1038/scientificamerican0599-40.

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45

Centrella, Joan, John Baker, Bernard Kelly, and James van Meter. "Merging black holes." Contemporary Physics 52, no. 1 (2011): 1–14. http://dx.doi.org/10.1080/00107514.2010.520908.

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46

Dvali, Georgi. "Quantum black holes." Physics Today 68, no. 1 (2015): 38–43. http://dx.doi.org/10.1063/pt.3.2656.

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47

Psaltis, Dimitrios, and Feryal Özel. "Imaging black holes." Physics Today 71, no. 4 (2018): 70–71. http://dx.doi.org/10.1063/pt.3.3906.

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48

Carr, Bernard J., and Steven B. Giddings. "Quantum Black Holes." Scientific American 292, no. 5 (2005): 48–55. http://dx.doi.org/10.1038/scientificamerican0505-48.

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49

AHN, EUN-JOO, and MARCO CAVAGLIÀ. "COSMIC BLACK HOLES." International Journal of Modern Physics D 12, no. 09 (2003): 1699–704. http://dx.doi.org/10.1142/s0218271803004006.

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Production of high-energy gravitational objects is a common feature of gravitational theories. The primordial universe is a natural setting for the creation of black holes and other nonperturbative gravitational entities. Cosmic black holes can be used to probe physical properties of the very early universe which would usually require the knowledge of the theory of quantum gravity. They may be the only tool to explore thermalization of the early universe. Whereas the creation of cosmic black holes was active in the past, it seems to be negligible at the present epoch.

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50

Miller, M. Coleman. "Black holes revealed." Physics World 23, no. 07 (2010): 36–37. http://dx.doi.org/10.1088/2058-7058/23/07/35.

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