Relevant bibliographies by topics / Calculation of black hole

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  1. Journal articles
  2. Dissertations / Theses
  3. Books
  4. Book chapters
  5. Conference papers
  6. Reports

Academic literature on the topic 'Calculation of black hole'

Author: Grafiati
Published: 4 June 2025
Last updated: 1 August 2025

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Journal articles on the topic "Calculation of black hole"

1

Padilla, Nelson D., Ignacio J. Araya, and Federico Stasyszyn. "The electric charge of black holes within galaxies." Journal of Cosmology and Astroparticle Physics 2024, no. 05 (2024): 044. http://dx.doi.org/10.1088/1475-7516/2024/05/044.

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Abstract We present improved estimates of the electric charge that black holes could hold when these are embedded in the ionised plasma within galaxies. We have implemented the spontaneous emission of charges of opposite sign to that of the black hole via athermal Hawking evaporation, including its dependence on black hole spin, and we have estimated the equilibrium charge that arises as this charge loss is balanced by the continuous accretion of charges from the surrounding plasma. The resulting charge can be several orders of magnitude lower than previously estimated upper limits, but it can
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Franciolini, G., A. Ianniccari, A. Kehagias, D. Perrone, and A. Riotto. "Renormalized primordial black holes." Journal of Cosmology and Astroparticle Physics 2024, no. 11 (2024): 001. http://dx.doi.org/10.1088/1475-7516/2024/11/001.

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Abstract The formation of primordial black holes in the early universe may happen through the collapse of large curvature perturbations generated during a non-attractor phase of inflation or through a curvaton-like dynamics after inflation. The fact that such small-scale curvature perturbation is typically non-Gaussian leads to the renormalization of composite operators built up from the smoothed density contrast and entering in the calculation of the primordial black abundance. Such renormalization causes the phenomenon of operator mixing and the appearance of an infinite tower of local, non-
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Fan, Zefang, Yu Wang, and Xianggao Wang. "Stability Analysis of Stable Circular Orbit in Multi-Static Black Hole Spacetime." Symmetry 16, no. 9 (2024): 1140. http://dx.doi.org/10.3390/sym16091140.

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We herein study the circular orbit stability of a static black hole system composed of multiple Reissner–Nordstrom (RN) black holes. By comparing the circular orbits of two static black holes, three static black holes (TBHs), four static black holes and five static black holes at different spacetime, we find that the continuity of their stable circular orbits changes, i.e., the peaks of the effective potentials are transformed from single-peaked to bi-peaked, and that the distance a between the black holes is the main reason for this change. This characteristic is completely different from the
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Sinha, Aloke Kumar. "Fluctuating quasi-stable quantum-charged rotating black holes." Modern Physics Letters A 35, no. 16 (2020): 2050136. http://dx.doi.org/10.1142/s0217732320501369.

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We are engaged in studying thermodynamics of black holes from quantum mechanical perspective and already have published a series of papers. We first showed, based on certain assumptions for quantum mechanical nature of black holes, that they can be thought to be immersed in a thermal bath, i.e. rest of the universe. Of course, this consideration is required to study the thermodynamics of the black holes. We were able to find out the conditions of thermal stability for a black hole with arbitrary number of hairs in arbitrary dimensional spacetime. They came in form of a series of inequalities,
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Liu, Chengyu, Minxing Wang, Guanxing Yi, and Yi Zhuang. "A Study on the logarithm correction of black hole entropy." Journal of Physics: Conference Series 2083, no. 2 (2021): 022042. http://dx.doi.org/10.1088/1742-6596/2083/2/022042.

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Abstract The logarithm correction of black hole entropy is important in understanding the essence of black hole entropy, providing a more accurate entropy calculation. We reviewed the mainstream method of logarithm correction of black hole entropy, including quantum loop gravity correction, conformal field theory correction, and classical thermal correction. Specifically, the correction of quantum loop gravity presents a stable general expression of logarithm correction, which only depends on the surface area of the black hole and solves the problem of meaningless entropy solution under a larg
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Qiu, Jiawei. "Misalignment of jet, orbital plane, and accretion disk observed in black hole binaries." Theoretical and Natural Science 31, no. 1 (2024): 256–61. http://dx.doi.org/10.54254/2753-8818/31/20241148.

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Black holes are interesting objects and prove to be the leading edge of testing and verifying of our understandings in gravity. Among some of the most sought after quantities is the spin of the black hole: it is closely related to how the black hole system behaves. Various attempts have been made to derive the spin of black holes, in which the orientation in space could be deduced using the spectrum produced by the accretion disk, observation of the jets produced by black holes, and calculation of the orbit of black hole binaries using light and velocity curves. These observations, however, ca
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SUN, XUEFENG, and WENBIAO LIU. "IMPROVED BLACK HOLE ENTROPY CALCULATION WITHOUT CUTOFF." Modern Physics Letters A 19, no. 09 (2004): 677–80. http://dx.doi.org/10.1142/s0217732304013192.

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The brick wall model and thin film model are most representative models in black hole entropy calculation. However, each of them must have a cutoff in order to avoid the divergence, and the divergence itself cannot be explained satisfactorily. Li Xiang6 substituted the classical uncertainty relation with the generalized uncertainty relation, the divergence was removed, consequently the cutoff was also removed. But due to the complex expression, he did not give the final solution. He only drew a conclusion that the upper bound of a black hole entropy is in proportional to its horizon area. The
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Sahlmann, Hanno. "Entropy calculation for a toy black hole." Classical and Quantum Gravity 25, no. 5 (2008): 055004. http://dx.doi.org/10.1088/0264-9381/25/5/055004.

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Bhattacharya, Prosad. "Calculation of the TOV Limit Based on Neutron Degeneracy Pressure." Indian Journal of Advanced Physics 4, no. 1 (2024): 4–7. http://dx.doi.org/10.54105/ijap.b1050.04010424.

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Original theory on the mass limit beyond which a cold, non-rotating neutron star cannot be formed, instead only stellar black holes will be created, was stipulated by J.R. Oppenheimer and G.M. Volkoff based on R.C. Tolman’s work in 1939. The limit calculated from the equation established by them is known as the TOV limit which is analogous to the Chandrasekhar limit for White Dwarfs. But the results obtained using the formula was found to be not valid today. Subsequent theoretical works place the limit in the range 1.5 to 3 solar masses. There are several basic theories and related formulae fo
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Situmorang, Adi Suarman, Juli Antasari Br Sinaga, Ratna Rintaningrum, and Ruben Cornelius Siagian. "Non-Linear Force Dynamics in Black Hole Accretion Disks Using Logarithmic and Trigonometric Approximations." Jurnal Penelitian Pendidikan IPA 11, no. 2 (2025): 988–1000. https://doi.org/10.29303/jppipa.v11i2.10291.

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Accretion disks are material structures that form when gas, dust or plasma is pulled towards a black hole by its strong gravity. In rotating (Kerr) black holes, the dynamics of the accretion disk becomes more complex due to frame-dragging effects that affect particle trajectories and energy release patterns. This study aims to develop an algorithm for calculating the force F(x) on particles in the accretion disk by considering the non-linear interaction between the black hole spin parameter and the relative position of the particles. The developed algorithm uses logarithmic and trigonometric a
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Dissertations / Theses on the topic "Calculation of black hole"

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Nielsen, Alex. "Black Hole Horizons and Black Hole Thermodynamics." Thesis, University of Canterbury. Physics and Astronomy, 2007. http://hdl.handle.net/10092/1363.

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This work investigates how black holes can be described in terms of different definitions of horizons. Global definitions in terms of event horizons and Killing horizons are contrasted with local definitions in terms of trapping horizons and dynamical horizons. The discussion is framed in the context of the laws of black hole thermodynamics.
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Galstyan, Irina. "Black-Hole Universe." Licentiate thesis, Stockholms universitet, Fysikum, 2017. http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-149311.

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In this contribution, we have constructed new analytical solutions for initial data of the Einstein equations. Such solutions are valuable for gaining a better understanding of problems involving strong gravitational and/or electromagnetic interactions in general relativity. In this process, we have examined an inhomogeneous cosmological model consisting a lattice of regularly arranged, charged black holes with initial data corresponding to the maximum expansion of a cosmological solution. We have also refined the method in such a way that the values of the mass and charge of the sources can b
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Ross, Simon Frederick. "Black hole pair creation." Thesis, University of Cambridge, 1996. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.627545.

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Hayakawa, Tomoyasu. "Black-Hole forming Supernovae." Kyoto University, 2020. http://hdl.handle.net/2433/253091.

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Chung, Hyeyoun. "Exploring Black Hole Dynamics." Thesis, Harvard University, 2014. http://nrs.harvard.edu/urn-3:HUL.InstRepos:14226081.

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This thesis explores the evolution of different types of black holes, and the ways in which black hole dynamics can be used to answer questions about other physical systems. We first investigate the differences in observable gravitational effects between a four-dimensional Randall-Sundrum (RS) braneworld universe compared to a universe without the extra dimension, by considering a black hole solution to the braneworld model that is localized on the brane. When the brane has a negative cosmological constant, then for a certain range of parameters for the black hole, the intersection of the bl
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Martínez, Montero Marina. "Studies of Black Hole Horizons." Doctoral thesis, Universitat de Barcelona, 2016. http://hdl.handle.net/10803/396271.

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This thesis has focused entirely on classical and thermodynamical aspects of black hole physics. We have developed four different projects involving different kinds of black holes. 1 BLACK BRANES IN A BOX Neutral black branes with extended horizons are dynamically unstable to long wavelength perturbations along their horizons; this instability is known as the Gregory-Laflamme instability. In some regimes, the dynamics of black branes can be captured by an effective hydrodynamic description. We have studied the effective hydrodynamics of neutral black branes inside a cylindrical cavity to i
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Costa, Joao Lopes. "On black hole uniqueness theorems." Thesis, University of Oxford, 2010. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.514963.

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Morsink, Sharon Marijke. "The generic black hole singularity." Thesis, National Library of Canada = Bibliothèque nationale du Canada, 1997. http://www.collectionscanada.ca/obj/s4/f2/dsk3/ftp04/nq21606.pdf.

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Klein-Wolt, Marc. "Black hole X-ray binaries." [S.l. : Amsterdam : s.n.] ; Universiteit van Amsterdam [Host], 2004. http://dare.uva.nl/document/91386.

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Ahmadi, Morteza, and University of Lethbridge Faculty of Arts and Science. "Aspects of black hole physics." Thesis, Lethbridge, Alta. : University of Lethbridge, Faculty of Arts and Science, 2006, 2006. http://hdl.handle.net/10133/386.

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In this thesis, aspects of the physics of black holes are reviewed and new results in black hole thermodynamics are presented. First, general black hole solutions of Einstein’s equations of general relativity are mentioned and a proof of conservation law of energy and momentum in general relativity is presented. Aspects of the laws of black hole mechanics and Hawking radiation are then studied. Two proposals which attempt to explain the origin of black hole entropy (the brick wall model and entanglement entropy) are then discussed. Finally, some recent work related to the possible production a
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Books on the topic "Calculation of black hole"

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Burns, Charles. Black Hole. Pantheon Books, 2005.

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Punsly, Brian. Black Hole Gravitohydromagnetics. Springer Berlin Heidelberg, 2001.

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Gill, David Macinnis. Black hole sun. Greenwillow Books, 2010.

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Frolov, Valeri P., and Igor D. Novikov. Black Hole Physics. Springer Netherlands, 1998. http://dx.doi.org/10.1007/978-94-011-5139-9.

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Meier, David L. Black Hole Astrophysics. Springer Berlin Heidelberg, 2012. http://dx.doi.org/10.1007/978-3-642-01936-4.

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Punsly, Brian. Black Hole Gravitohydromagnetics. Springer Berlin Heidelberg, 2009. http://dx.doi.org/10.1007/978-3-540-76957-6.

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Sabbata, Venzo, and Zhenjiu Zhang, eds. Black Hole Physics. Springer Netherlands, 1992. http://dx.doi.org/10.1007/978-94-011-2420-1.

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Punsly, Brian. Black Hole Gravitohydromagnetics. Springer Berlin Heidelberg, 2001. http://dx.doi.org/10.1007/978-3-662-04409-4.

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Day, Gerry, Gary Nelson, Ron Miller, and Jeb Rosebrook. The black hole. Walt Disney Home Video, 2004.

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Grumiller, Daniel, and Mohammad Mehdi Sheikh-Jabbari. Black Hole Physics. Springer International Publishing, 2022. http://dx.doi.org/10.1007/978-3-031-10343-8.

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Book chapters on the topic "Calculation of black hole"

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Duplij, Steven, Joshua Feinberg, Moshe Moshe, et al. "Black Hole." In Concise Encyclopedia of Supersymmetry. Springer Netherlands, 2004. http://dx.doi.org/10.1007/1-4020-4522-0_64.

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Prantzos, Nikos. "Black Hole." In Encyclopedia of Astrobiology. Springer Berlin Heidelberg, 2015. http://dx.doi.org/10.1007/978-3-662-44185-5_199.

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Prantzos, Nikos. "Black Hole." In Encyclopedia of Astrobiology. Springer Berlin Heidelberg, 2011. http://dx.doi.org/10.1007/978-3-642-11274-4_199.

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Prantzos, Nikos. "Black Hole." In Encyclopedia of Astrobiology. Springer Berlin Heidelberg, 2014. http://dx.doi.org/10.1007/978-3-642-27833-4_199-3.

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Bentivegna, Eloisa. "Black-Hole Lattices." In Progress in Mathematical Relativity, Gravitation and Cosmology. Springer Berlin Heidelberg, 2013. http://dx.doi.org/10.1007/978-3-642-40157-2_13.

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Frolov, Valeri. "Black Hole Entropy." In Quantum Field Theory Under the Influence of External Conditions. Vieweg+Teubner Verlag, 1996. http://dx.doi.org/10.1007/978-3-663-01204-7_34.

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Bona, Carles, Carles Bona-Casas, and Carlos Palenzuela-Luque. "Black Hole Simulations." In Elements of Numerical Relativity and Relativistic Hydrodynamics. Springer Berlin Heidelberg, 2009. http://dx.doi.org/10.1007/978-3-642-01164-1_6.

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Novikov, Igor D., and Valery P. Frolov. "Rotating Black Hole." In Physics of Black Holes. Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-017-2651-1_4.

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Novikov, Igor D., and Valery P. Frolov. "Black-Hole Electrodynamics." In Physics of Black Holes. Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-017-2651-1_7.

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Duplij, Steven, Joshua Feinberg, Moshe Moshe, et al. "Black Hole Entropy." In Concise Encyclopedia of Supersymmetry. Springer Netherlands, 2004. http://dx.doi.org/10.1007/1-4020-4522-0_65.

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Conference papers on the topic "Calculation of black hole"

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Barath Ramesh, R., and S. John Justin Thangaraj. "Black Hole Attack Detection in Adhoc Networks Using KNN Algorithm with Reputation Calculation." In 2023 4th International Conference on Smart Electronics and Communication (ICOSEC). IEEE, 2023. http://dx.doi.org/10.1109/icosec58147.2023.10276377.

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Yo, Hwei-Jang. "Improved numerical stability of rotating black hole evolution calculations." In Proceedings of the VII Asia-Pacific International Conference. WORLD SCIENTIFIC, 2006. http://dx.doi.org/10.1142/9789812772923_0005.

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Centrella, Joan M. "Calculating Gravitational Wave Signatures from Binary Black Hole Mergers." In THE ASTROPHYSICS OF GRAVITATIONAL WAVE SOURCES. AIP, 2003. http://dx.doi.org/10.1063/1.1629434.

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KABAT, DANIEL, GILAD LIFSCHYTZ, and DAVID LOWE. "BLACK HOLE THERMODYNAMICS FROM CALCULATIONS IN STRONGLY COUPLED GAUGE THEORY." In Proceedings of the 2000 International Superstrings Conference. WORLD SCIENTIFIC, 2001. http://dx.doi.org/10.1142/9789812810328_0019.

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Ipatov, S. "Migration of planetesimals in the TRAPPIST-1 exoplanetary system." In Modern astronomy: from the Early Universe to exoplanets and black holes. Special Astrophysical Observatory of the Russian Academy of Sciences, 2024. https://doi.org/10.26119/vak2024.135.

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The calculations of the motion of planetesimals at the late stages of accumulation of planets in the TRAPPIST-1 system were made. In each calculation variant, initial orbits of planetesimals were near one of the planets. The number of collisions of planetesimals with the planets were calculated. The calculations has shown that the outer layers of neighboring exoplanets in the TRAPPIST-1 system can include similar material if there were a lot of planetesimals near their orbits at the late stages of the accumulation of the exoplanets.
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Sa̧dowski, Aleksander, Janusz Ziółkowski, Krzysztof Belczyński, et al. "Calculations of the Galactic Population of Black Hole X-Ray Binaries." In A POPULATION EXPLOSION: The Nature & Evolution of X-ray Binaries in Diverse Environments. AIP, 2008. http://dx.doi.org/10.1063/1.2945086.

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Khoperskov, A., S. Khrapov, D. Sirotin, and A. Zasov. "Merging of spiral galaxies: observations and modeling." In Modern astronomy: from the Early Universe to exoplanets and black holes. Special Astrophysical Observatory of the Russian Academy of Sciences, 2024. https://doi.org/10.26119/vak2024.025.

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We present a study of the dynamics of multi-component models of spiral galaxies at different stages of grand mergers. The numerical models include a self-consistent account of the dynamics of collisionless stellar subsystems and N-body dark matter, as well as gaseous components. The calculation of gas heating and cooling processes allows us to consider a wide temperature range from 80 to 100 thousand degrees. The use of the method of Smoothed-particle hydrodynamics to solve the hydrodynamic equations makes it possible to follow the evolution of the gas of each galaxy, calculating the content o
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Faber, Joshua A., Thomas W. Baumgarte, Stuart L. Shapiro, Keisuke Taniguchi, and Frederic A. Rasio. "Black Hole-Neutron Star Binary Merger Calculations: GRB Progenitors and the Stability of Mass Transfer." In ALBERT EINSTEIN CENTURY INTERNATIONAL CONFERENCE. AIP, 2006. http://dx.doi.org/10.1063/1.2399634.

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Chmyreva, Elizaveta, and G. Beskin. "On the detection of emission near the event horizons of accreting stellar-mass black holes." In Modern astronomy: from the Early Universe to exoplanets and black holes. Special Astrophysical Observatory of the Russian Academy of Sciences, 2024. https://doi.org/10.26119/vak2024.010.

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We discuss the possibility of detecting signs of the existence of stellar-mass black hole (BH) event horizons in the emission of interstellar gas accreting on them. We consider a sample of invisible compact objects detected as companions of Main Sequence stars in wide binaries. Theoretical luminosities and accretion rates of the interstellar gas were obtained within the framework of the spherical accretion model. BH velocities estimated from binary system dynamics, as well as the density of the surrounding ISM, were used in the calculations. Based on the sensitivity data of existing and projec
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Kondratieva, T. "Evolution of non-spherical porous dust grains in galaxies." In Modern astronomy: from the Early Universe to exoplanets and black holes. Special Astrophysical Observatory of the Russian Academy of Sciences, 2024. https://doi.org/10.26119/vak2024.066.

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Recent research has examined the evolution of interstellar dust grain size distribution over time scales of up to 10 Gyr, focusing on the primary grain growth and destruction mechanisms present in both the diffuse and dense interstellar medium. The grains were modeled as porous spheres, and for the first time, the porosity was considered to depend on the particle size and time. In this work, it is proposed in the first approximation that non-spherical dust grains have a comparable mass distribution to that of spherical ones. The use of porous spheroids facilitates the calculation of the time e
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Reports on the topic "Calculation of black hole"

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Lim, Hyun. Safe Travel Guide to Black Hole. Office of Scientific and Technical Information (OSTI), 2020. http://dx.doi.org/10.2172/1603963.

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Dabholkar, A. Exact Counting of Black Hole Microsates. Office of Scientific and Technical Information (OSTI), 2004. http://dx.doi.org/10.2172/839944.

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Chen, Pisin. Black Hole Remnants and Dark Matter. Office of Scientific and Technical Information (OSTI), 2002. http://dx.doi.org/10.2172/799976.

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Hsu, Jonathan P., Alexander Maloney, and Alessandro Tomasiello. Black Hole Attractors and Pure Spinors. Office of Scientific and Technical Information (OSTI), 2006. http://dx.doi.org/10.2172/876603.

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Ortega-Rodriguez, Manuel, Appl Phys Dept /Costa Rica U. /Stanford U., Alexander S. Silbergleit, HEPL /Stanford U., Robert V. Wagoner, and Phys Dept /KIPAC, Menlo Park /Stanford U. Normal Modes of Black Hole Accretion Disks. Stanford Linear Accelerator Center (SLAC), 2006. http://dx.doi.org/10.2172/894930.

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Rodriguez, C., G. B. Taylor, R. T. Zavala, A. B. Peck, L. K. Pollack, and R. W. Romani. A Compact Supermassive Binary Black Hole System. Defense Technical Information Center, 2006. http://dx.doi.org/10.21236/ada446245.

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Kollosh, R. The Non-BPS Black Hole Attractor Equation. Office of Scientific and Technical Information (OSTI), 2006. http://dx.doi.org/10.2172/876040.

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Kinch, Brooks. Analyzing Black Hole X-Rays with Simulations. Office of Scientific and Technical Information (OSTI), 2021. http://dx.doi.org/10.2172/1768430.

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Chen, Pisin. The Generalized Uncertainty Principle and Black Hole Remnants. Office of Scientific and Technical Information (OSTI), 2001. http://dx.doi.org/10.2172/784935.

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Liedahl, D., and C. Mauche. Structure and Spectroscopy of Black Hole Accretion Disks. Office of Scientific and Technical Information (OSTI), 2005. http://dx.doi.org/10.2172/918406.

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