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Artykuły w czasopismach na temat „Black holes”

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Autor: Grafiati

Data publikacji: 4 czerwca 2021

Data aktualizacji: 29 lipca 2024

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1

Krauss, Lawrence M., Hong Liu i Junseong Heo. "Dirty Black Holes and Hairy Black Holes". Physical Review Letters 77, nr 26 (23.12.1996): 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, nr 4778 (14.11.1986): 882. http://dx.doi.org/10.1126/science.234.4778.882.

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3

Rovelli, Carlo. "Black holes". Europhysics News 52, nr 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, nr 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, nr 5 (maj 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, nr 1-4 (styczeń 2003): 139–54. http://dx.doi.org/10.1080/01422410310001610464.

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7

Horowitz, Gary T., i Saul A. Teukolsky. "Black holes". Reviews of Modern Physics 71, nr 2 (1.03.1999): S180—S186. http://dx.doi.org/10.1103/revmodphys.71.s180.

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8

Brugmann, B., A. M. Ghez i J. Greiner. "Black holes". Proceedings of the National Academy of Sciences 98, nr 19 (11.09.2001): 10525–26. http://dx.doi.org/10.1073/pnas.201365798.

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9

Ferreira, Pedro. "Black holes". New Scientist 207, nr 2767 (lipiec 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, nr 1 (styczeń 1990): 35–49. http://dx.doi.org/10.1016/0364-9229(90)90010-x.

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11

Creighton, Teviet, i Richard Price. "Black holes". Scholarpedia 3, nr 1 (2008): 4277. http://dx.doi.org/10.4249/scholarpedia.4277.

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12

Karouzos, Marios. "Black holes". Nature Astronomy 3, nr 1 (styczeń 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, nr 4 (2014): 77–91. http://dx.doi.org/10.1353/aph.2014.0087.

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14

Zaslavskii, O. B. "Truly naked black holes and quasi-black holes". Gravitation and Cosmology 14, nr 1 (styczeń 2008): 60–64. http://dx.doi.org/10.1134/s0202289308010088.

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15

Lifschytz, Gilad. "Charged black holes from near extremal black holes". Journal of High Energy Physics 2004, nr 09 (8.09.2004): 009. http://dx.doi.org/10.1088/1126-6708/2004/09/009.

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16

Grib, A. A. "Are black holes black?" Soviet Physics Journal 32, nr 5 (maj 1989): 401–3. http://dx.doi.org/10.1007/bf00895326.

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17

Haldar, Amritendu, i Ritabrata Biswas. "Thermodynamic studies of different type of black holes: General uncertainty principle approach". Modern Physics Letters A 33, nr 34 (7.11.2018): 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 the black holes and interpret them physically. We depict a comparative study of thermodynamics between the aforesaid types of black holes. We find the existence of a transition of phase. Finally, we obtain the quantum corrected thermodynamics on the basis of general uncertainty principle and it is seen from the quantum-corrected entropy that it contains the logarithmic term. We offer comparative studies on joint effect of generalized uncertainty principle parameter [Formula: see text] along with the concerned black holes’ parameters on the thermodynamics.

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18

Fishbach, Maya, Daniel E. Holz i Ben Farr. "Are LIGO's Black Holes Made from Smaller Black Holes?" Astrophysical Journal 840, nr 2 (11.05.2017): L24. http://dx.doi.org/10.3847/2041-8213/aa7045.

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19

Li, Miao. "Macroscopic black holes, microscopic black holes and noncommutative membrane". Classical and Quantum Gravity 21, nr 14 (29.06.2004): 3571–78. http://dx.doi.org/10.1088/0264-9381/21/14/016.

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20

Unruh, W. G. "Dumb holes: analogues for black holes". Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 366, nr 1877 (5.06.2008): 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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21

Courvoisier, T. J. L., i B. Wilkes. "High-Energy Radiation from Black Holes: From Supermassive Black Holes to Galactic Solar Mass Black Holes". Advances in Space Research 38, nr 7 (styczeń 2006): 1345. http://dx.doi.org/10.1016/j.asr.2006.06.001.

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22

Mu, Benrong, Peng Wang i 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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23

Grib, A. A., i Yu V. Pavlov. "Are black holes totally black?" Gravitation and Cosmology 21, nr 1 (styczeń 2015): 13–18. http://dx.doi.org/10.1134/s0202289315010065.

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24

Genzel, Reinhard. "How black holes stay black". Nature 391, nr 6662 (styczeń 1998): 17–18. http://dx.doi.org/10.1038/34029.

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25

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

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26

Hsu, Stephen D. H. "White holes and eternal black holes". Classical and Quantum Gravity 29, nr 1 (12.12.2011): 015004. http://dx.doi.org/10.1088/0264-9381/29/1/015004.

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27

Palchoudhury, Sankar. "About Black Holes". International Journal of Fundamental Physical Sciences 11, nr 1 (marzec 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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28

Steiner, George. "Some Black Holes". Bulletin of the American Academy of Arts and Sciences 41, nr 2 (listopad 1987): 12. http://dx.doi.org/10.2307/3822663.

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29

Aliev, A. N., i D. V. Gal'tsov. ""Magnetized" black holes". Uspekhi Fizicheskih Nauk 157, nr 1 (1989): 129. http://dx.doi.org/10.3367/ufnr.0157.198901d.0129.

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30

Dalton, Kenneth. "Supermassive Black Holes". Journal of High Energy Physics, Gravitation and Cosmology 05, nr 03 (2019): 984–88. http://dx.doi.org/10.4236/jhepgc.2019.53052.

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31

de Valk, Giliam. "Analytic Black Holes". National security and the future 23, nr 1 (3.02.2022): 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 analyses. Furthermore, hybrid threats and real time intelligence for the protection of the critical infrastructure demand a new approach towards analysis. This gap needs to be filled, among others, by data science cells that can process data automatically. This way, a new analytic approach can be reached – that of Augmented Intelligence – in which humans and machines are paired in the analytic process. Human Analysis is likely to develop more towards to limit the number of data taken into account, but those data will have a high causal significance. Machine Analysis, on the other hand, will process huge amount of data and focus on correlations in the first place. Augmented Intelligence, will be a merger of both, that can manifest itself by different combinations of both. It will deal with data that now remain unused. It can fill the gap of the identified analytic black holes. Dealing with the analytic black holes will enhance the security, and make us more effective in protecting our critical infrastructure.

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32

Shurcliff, William A. "Black Holes—"Ingestars"?" Science 231, nr 4744 (21.03.1986): 1355. http://dx.doi.org/10.1126/science.231.4744.1355.f.

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33

Bizon, Piotr. "Colored black holes". Physical Review Letters 64, nr 24 (11.06.1990): 2844–47. http://dx.doi.org/10.1103/physrevlett.64.2844.

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34

de Freitas Pacheco, José Antonio. "Dormant Black Holes". International Journal of Modern Physics: Conference Series 45 (styczeń 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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35

Ho, Pei-Ming. "Asymptotic black holes". Classical and Quantum Gravity 34, nr 8 (22.03.2017): 085006. http://dx.doi.org/10.1088/1361-6382/aa641e.

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36

Derbes, David. "Exploring Black Holes". American Journal of Physics 89, nr 1 (styczeń 2021): 121–23. http://dx.doi.org/10.1119/10.0002493.

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37

Buchanan, Mark. "Defining black holes". Nature Physics 14, nr 10 (październik 2018): 970. http://dx.doi.org/10.1038/s41567-018-0299-1.

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38

Zeng, Xiaoxiong, Christian Corda i 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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39

Lasota, Jean-Pierre. "Unmasking Black Holes". Scientific American 280, nr 5 (maj 1999): 40–47. http://dx.doi.org/10.1038/scientificamerican0599-40.

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40

Centrella, Joan, John Baker, Bernard Kelly i James van Meter. "Merging black holes". Contemporary Physics 52, nr 1 (styczeń 2011): 1–14. http://dx.doi.org/10.1080/00107514.2010.520908.

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41

Dvali, Georgi. "Quantum black holes". Physics Today 68, nr 1 (styczeń 2015): 38–43. http://dx.doi.org/10.1063/pt.3.2656.

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42

Psaltis, Dimitrios, i Feryal Özel. "Imaging black holes". Physics Today 71, nr 4 (kwiecień 2018): 70–71. http://dx.doi.org/10.1063/pt.3.3906.

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43

Carr, Bernard J., i Steven B. Giddings. "Quantum Black Holes". Scientific American 292, nr 5 (maj 2005): 48–55. http://dx.doi.org/10.1038/scientificamerican0505-48.

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44

AHN, EUN-JOO, i MARCO CAVAGLIÀ. "COSMIC BLACK HOLES". International Journal of Modern Physics D 12, nr 09 (październik 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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45

Miller, M. Coleman. "Black holes revealed". Physics World 23, nr 07 (lipiec 2010): 36–37. http://dx.doi.org/10.1088/2058-7058/23/07/35.

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46

Shaoul, Jean, Anne Stafford i Pam Stapleton. "Financial black holes". Accounting, Auditing & Accountability Journal 23, nr 2 (16.02.2010): 229–55. http://dx.doi.org/10.1108/09513571011023200.

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47

Horgan, John. "Bashing Black Holes". Scientific American 273, nr 1 (lipiec 1995): 16–17. http://dx.doi.org/10.1038/scientificamerican0795-16.

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48

BROUT, R., i PH SPINDEL. "Black holes dispute". Nature 337, nr 6204 (styczeń 1989): 215–16. http://dx.doi.org/10.1038/337215c0.

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49

GUNZIG, E. "Black holes dispute". Nature 337, nr 6204 (styczeń 1989): 216. http://dx.doi.org/10.1038/337216a0.

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50

Ferrarese, Laura, i David Merritt. "Supermassive black holes". Physics World 15, nr 6 (czerwiec 2002): 41–46. http://dx.doi.org/10.1088/2058-7058/15/6/43.

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