Literatura académica sobre el tema "Vaidya’s black hole"
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Artículos de revistas sobre el tema "Vaidya’s black hole"
IBOHAL, NG y L. KAPIL. "CHARGED BLACK HOLES IN VAIDYA BACKGROUNDS: HAWKING'S RADIATION". International Journal of Modern Physics D 19, n.º 04 (abril de 2010): 437–64. http://dx.doi.org/10.1142/s0218271810016518.
Texto completoIBOHAL, NG y L. DORENDRO. "NON-STATIONARY ROTATING BLACK HOLES: ENTROPY AND HAWKING'S RADIATION". International Journal of Modern Physics D 14, n.º 08 (agosto de 2005): 1373–412. http://dx.doi.org/10.1142/s0218271805007127.
Texto completoMustari, Mustari y Yuant Tiandho. "Thermodynamics of a Non-Stationary Black Hole Based on Generalized Uncertainty Principle". Journal of Physics: Theories and Applications 1, n.º 2 (29 de octubre de 2017): 127. http://dx.doi.org/10.20961/jphystheor-appl.v1i2.19308.
Texto completoLIU, BAI SHENG y JING YI ZHANG. "DISCUSSION ON EVENT HORIZON AND QUANTUM ERGOSPHERE OF DYNAMIC DE SITTER BLACK HOLES". Modern Physics Letters A 27, n.º 04 (10 de febrero de 2012): 1250010. http://dx.doi.org/10.1142/s0217732312500101.
Texto completoCASTRO, C., J. A. NIETO, L. RUIZ y J. SILVAS. "ON TIME-DEPENDENT BLACK HOLES AND COSMOLOGICAL MODELS FROM A KALUZA–KLEIN MECHANISM". International Journal of Modern Physics A 24, n.º 07 (20 de marzo de 2009): 1383–415. http://dx.doi.org/10.1142/s0217751x09042931.
Texto completoIshwarchandray, Ngangbam y Ng Ibohal. "Black Holes in Non-stationary de Sitter Space with Variable Λ(u)". Journal of the Tensor Society 11, n.º 01 (30 de junio de 2007): 25–48. http://dx.doi.org/10.56424/jts.v11i01.10586.
Texto completoWU, S. Q. y X. CAI. "NON-EXISTENCE OF NEW QUANTUM ERGOSPHERE EFFECT OF A VAIDYA-TYPE BLACK HOLE". Modern Physics Letters A 16, n.º 24 (10 de agosto de 2001): 1549–57. http://dx.doi.org/10.1142/s0217732301004789.
Texto completoKumah, Mohammed y Francis T. Oduro. "On the Trapped Surface Characterization of Black Hole Region in Vaidya Spacetime". Journal of Mathematics Research 10, n.º 1 (8 de enero de 2018): 59. http://dx.doi.org/10.5539/jmr.v10n1p59.
Texto completoChen, Ge-Rui y Yong-Chang Huang. "Entropy spectrum of the apparent horizon of Vaidya black holes via adiabatic invariance". Modern Physics Letters A 31, n.º 06 (21 de febrero de 2016): 1650011. http://dx.doi.org/10.1142/s0217732316500115.
Texto completoSadeghian, S. y A. Shafiekhani. "Extremal charged Vaidya and its near horizon geometry". International Journal of Modern Physics D 26, n.º 04 (17 de febrero de 2017): 1750036. http://dx.doi.org/10.1142/s0218271817500365.
Texto completoTesis sobre el tema "Vaidya’s black hole"
Coudray, Armand. "Asymptotic behaviour of zero rest-mass fields on radiative space-times". Electronic Thesis or Diss., Brest, 2024. http://www.theses.fr/2024BRES0026.
Texto completoThis thesis adresses two distinct subjects. The first part examines the asymptotic behavior of scalar waves in the Vaidya spacetime, describing a spherical white hole evaporating via emission of isotropic dust. The analysis focuses on the regularity of conformal scalar waves at the isotropic boundary (past and future) of the compactified spacetime, depending on the initial data of the conformal field. Additionally, we construct the conformal scattering operator, demonstrating its ability to encode the entire field evolution in the compactified spacetime.These findings rely on energy inequalities and vector field methods.The second part centers on analyzing incoming isotropic curves in the purely radiative Robinson-Trautman spacetimes of type D. In contrast to a previous study on Vaidya’s metric, these curves do not form the past horizon due to the solution’s geometry. The final chapter categorizes these curves, revealing a behavior akin to that observed in Vaidya’s spacetime
Rossi, Dario. "Reissner-Nordström black holes and mass inflation". Bachelor's thesis, Alma Mater Studiorum - Università di Bologna, 2019. http://amslaurea.unibo.it/18370/.
Texto completoChirenti, Cecilia Bertoni Martha Hadler. "Perturbações de sistemas gravitacionais: a métrica de vaidya, mini buracos negros e gravastares". Universidade de São Paulo, 2007. http://www.teses.usp.br/teses/disponiveis/43/43134/tde-12092007-152702/.
Texto completoPerturbative studies of gravitational systems in General Relativity have gone through big developments in the last years, especially due to the evolution of the modern gravitational wave detectors. We consider in this work different perturbations in different scenarios. Firstly we consider the Vaidya metric, mainly used to describe time-dependent spherically symmetric spacetimes. Our simulations show that the frequencies of the quasinormal modes (QNM\'s) present a new inertial effect for rapidly varying mass functions, returning afterwards to the adiabatic behavior. Next we present a model for evaporating mini black holes in particle accelerators, in the context of the new gravity models with extra dimensions. With our model, based on the n-dimensional Vaidya metric, we are able to perform a QNM analysis which results in the possibility of obtaining the parameters of the black hole, such as its initial mass and the number of extra dimensions, from the experimental measurements. Finally, we present a study of a new solution, the gravastar, proposed as an alternative model for the end state of massive stars. We obtain bounds for the parameters of the solution and verify its stability against axial perturbations. Our results indicate that the gravastar\'s QNM spectrum can indeed be used to distinguish a black hole from a gravastar.
Actas de conferencias sobre el tema "Vaidya’s black hole"
Triyanta, H. M. Siahaan y A. N. Bowaire. "Hawking temperatures for the Vaidya and the Reissner-Nordstrom-Vaidya black holes". En THE 4TH INTERNATIONAL CONFERENCE ON THEORETICAL AND APPLIED PHYSICS (ICTAP) 2014. AIP Publishing LLC, 2016. http://dx.doi.org/10.1063/1.4943704.
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