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Thematische Bibliographien / Relativistic compact objects

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Auswahl der wissenschaftlichen Literatur zum Thema „Relativistic compact objects“

Autor: Grafiati

Veröffentlicht am 18. Mai 2024

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Zeitschriftenartikel zum Thema "Relativistic compact objects"

1

Mizuno, Yosuke. „GRMHD Simulations and Modeling for Jet Formation and Acceleration Region in AGNs“. Universe 8, Nr. 2 (28.01.2022): 85. http://dx.doi.org/10.3390/universe8020085.

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Relativistic jets are collimated plasma outflows with relativistic speeds. Astrophysical objects involving relativistic jets are a system comprising a compact object such as a black hole, surrounded by rotating accretion flows, with the relativistic jets produced near the central compact object. The most accepted models explaining the origin of relativistic jets involve magnetohydrodynamic (MHD) processes. Over the past few decades, many general relativistic MHD (GRMHD) codes have been developed and applied to model relativistic jet formation in various conditions. This short review provides an overview of the recent progress of GRMHD simulations in generating relativistic jets and their modeling for observations.

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Paul, Bikash Chandra, und Rumi Deb. „Relativistic solutions of anisotropic compact objects“. Astrophysics and Space Science 354, Nr. 2 (13.09.2014): 421–30. http://dx.doi.org/10.1007/s10509-014-2097-2.

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3

Mak, M. K., und T. Harko. „Relativistic compact objects in isotropic coordinates“. Pramana 65, Nr. 2 (August 2005): 185–92. http://dx.doi.org/10.1007/bf02898610.

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4

Mitra, Abhas, und Krishna Kumar Singh. „Thermal Radiation from Compact Objects in Curved Space-Time“. Universe 8, Nr. 10 (26.09.2022): 504. http://dx.doi.org/10.3390/universe8100504.

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We highlight here the fact that the distantly observed luminosity of a spherically symmetric compact star radiating thermal radiation isotropically is higher by a factor of (1+zb)2 compared to the corresponding flat space-time case, where zb is the surface gravitational redshift of the compact star. In particular, we emphasize that if the thermal radiation is indeed emitted isotropically along the respective normal directions at each point, this factor of increment (1+zb)2 remains unchanged even if the compact object would lie within its photon sphere. Since a canonical neutron star has zb≈0.1, the actual X-ray luminosity from the neutron star surface could be ∼20% higher than what would be interpreted by ignoring the general relativistic effects described here. For a static compact object, supported by only isotropic pressure, compactness is limited by the Buchdahl limit zb<2.0. However, for compact objects supported by anisotropic pressure, zb could be even higher (zb<5.211). In addition, in principle, there could be ultra-compact objects having zb≫1. Accordingly, the general relativistic effects described here might be quite important for studies of thermal radiation from some ultra-compact objects.

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EKŞİ, Kazım Yavuz. „Neutron stars: compact objects with relativistic gravity“. TURKISH JOURNAL OF PHYSICS 40 (2016): 127–38. http://dx.doi.org/10.3906/fiz-1510-11.

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CHATTOPADHYAY, PRADIP KUMAR, RUMI DEB und BIKASH CHANDRA PAUL. „RELATIVISTIC SOLUTION FOR A CLASS OF STATIC COMPACT CHARGED STAR IN PSEUDO-SPHEROIDAL SPACETIME“. International Journal of Modern Physics D 21, Nr. 08 (August 2012): 1250071. http://dx.doi.org/10.1142/s021827181250071x.

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Considering Vaidya–Tikekar metric, we obtain a class of solutions of the Einstein–Maxwell equations for a charged static fluid sphere. The physical 3-space (t = const. ) here is described by pseudo-spheroidal geometry. The relativistic solution for the theory is used to obtain models for charged compact objects; thereafter, a qualitative analysis of the physical aspects of compact objects are studied. The dependence of some of the properties of a superdense star on the parameters of the three geometry is explored. We note that the spheroidicity parameter a plays an important role for determining the properties of a compact object. A nonlinear equation of state (EOS) is required to describe a charged compact object with pseudo-spheroidal geometry, which we have shown for known masses of compact objects. We also note that the size of a static compact charged star is more than that of a static compact star without charge.

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Gallo, Emanuel, und Osvaldo M. Moreschi. „Modeling the dynamics of black holes through balanced equations of motion“. International Journal of Geometric Methods in Modern Physics 16, Nr. 03 (März 2019): 1950034. http://dx.doi.org/10.1142/s0219887819500348.

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We present a general approach for the formulation of equations of motion for astrophysical compact objects in general relativistic theories. The objects are modeled as relativistic particles, which are assumed to be moving in a geometric background which in turn is asymptotically flat. The background can be affected by the compact object; so that our approach can be applied to binary systems; by concentrating on the main contributions coming from back reaction effects due to gravitational radiation. Our premises are different from the traditional post-Newtonian and self-force approaches since we make strong use of the asymptotic properties of the self geometry of the particle; as is described below. In particular, we use a center of mass setting, and relativistic individual dynamical times for each object. We expect our model to complement the other approaches in different regimes.

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Sharif, M., und Arfa Waseem. „Charged compact objects in f(R,T) gravity“. International Journal of Modern Physics D 28, Nr. 02 (Januar 2019): 1950033. http://dx.doi.org/10.1142/s0218271819500330.

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This paper analyzes the effects of charge on the nature of relativistic compact star candidates with anisotropic distribution in the framework of [Formula: see text] gravity. For this purpose, we consider Krori–Barua solutions and obtain the values of unknown constants as well as charge using observational data of Her X-1, 4U1820-30 and SAX J 1808.4-3658 star models. For three viable [Formula: see text] models, we investigate the behavior of energy density, transverse as well as radial pressures in the interior geometry of these stars. The validity of energy conditions, effect of anisotropic factor and stability of these stellar models are also examined. We conclude that the effect of charge leads to more stable structures of relativistic compact objects.

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Chevalier, Roger A. „Compact Objects in Supernova Remnants“. International Astronomical Union Colloquium 145 (1996): 399–406. http://dx.doi.org/10.1017/s0252921100008253.

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Core collapse in very massive stars can lead to a central black hole that swallows the rest of the star and in less massive stars to a central neutron star and explosion. There is probably an intermediate mass range that gives an explosion and a central black hole; supernova remnants with no observable central object are candidates. The association of pulsars with Type II supernovae gives an estimate of the pulsar power to be expected in a supernova, but the uncertainty in the initial pulsar periods gives a wide range in possible powers. The relativistic wind bubble model for the Crab Nebula has steadily developed and there are now predictions regarding particle acceleration in the optical wisps. The bubble model with expansion into supernova gas can also be applied to other young pulsar nebulae.

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Tomimatsu, Akira. „Relativistic Dynamos in Magnetospheres of Rotating Compact Objects“. Astrophysical Journal 528, Nr. 2 (10.01.2000): 972–78. http://dx.doi.org/10.1086/308190.

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Dissertationen zum Thema "Relativistic compact objects"

1

Deb, Rumi. „Relativistic solutions of massive compact objects and stellar models in different space-time geometries“. Thesis, University of North Bengal, 2018. http://hdl.handle.net/123456789/2685.

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Völkel, Sebastian [Verfasser], und Kostas [Akademischer Betreuer] Kokkotas. „On the Gravitational Wave Spectrum of Compact Relativistic Objects / Sebastian Völkel ; Betreuer: Kostas Kokkotas“. Tübingen : Universitätsbibliothek Tübingen, 2020. http://d-nb.info/1212024931/34.

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Efremov, Pavel [Verfasser], Volker [Akademischer Betreuer] Perlick, Volker [Gutachter] Perlick und Domenico [Gutachter] Giulini. „Relativistic accretion onto compact objects / Pavel Efremov ; Gutachter: Volker Perlick, Domenico Giulini ; Betreuer: Volker Perlick“. Bremen : Staats- und Universitätsbibliothek Bremen, 2018. http://d-nb.info/1164151983/34.

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Schroven, Kris Inken [Verfasser], Claus [Akademischer Betreuer] Lämmerzahl, Claus [Gutachter] Lämmerzahl und Jutta [Gutachter] Kunz. „The Role of Electric Charge in Relativistic Accretion onto Compact Objects : an Analytical Approach / Kris Inken Schroven ; Gutachter: Claus Lämmerzahl, Jutta Kunz ; Betreuer: Claus Lämmerzahl“. Bremen : Staats- und Universitätsbibliothek Bremen, 2018. http://d-nb.info/1171420455/34.

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Giraud, Quentin. „Corrections général-relativistes à l’émission radio et haute énergie des pulsars“. Thesis, Strasbourg, 2020. http://www.theses.fr/2020STRAE024.

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Les étoiles à neutrons sont des astres extrêmement denses, plus denses qu’un noyau atomique, formés au cours d’une supernova. Un étoile à neutrons typique concentre ainsi une masse supérieure à celle du Soleil dans son diamètre d’une vingtaine de kilomètres. D’après la théorie de la relativité générale, qui décrit la gravité comme une déformation de l’espace-temps, le champ gravitationnel de ces étoiles devrait affecter de manière non négligeable les rayonnements électromagnétiques à proximité de celles-ci. Au cours de ma thèse, j’ai simulé les émissions radio et haute énergie provenant de l’accélération de particules le long des lignes de champ magnétique d’une étoile à neutrons dans la métrique de Schwarzschild pour savoir comment le rayonnement ainsi produit allait être affecté par les déformations de l’espace-temps au voisinage de l’étoile à neutrons
Neutron stars are very dense objects, denser than an atomic nucleus, formed during a supernova. A typical neutron star concentrates a mass superior to the one of the Sun in its diameter of around twenty kilometers. According to general relativity, which describes gravity as a space-time distorsion, the gravitational field of those stars should have a non-negligible impact on electromagnetic radiations close to them. During my thesis, I have simulated radio and high-energy emission originating from particules accelerated along the magnetic field lines of the neutron star inside the Schwarzschild metric to have an insight of how this kind of radiations would be affected by space-time distorsions in the vicinity of the neutron star

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Luz, Paulo Miguel Grilo da. „Compact objects, gravitational collapse and singularities in relativistic theories of gravitation“. Doctoral thesis, 2020. http://hdl.handle.net/1822/76574.

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Programa doutoral em Física (MAP-fis)
A natureza e a evolução de objetos astrofísicos massivos providenciam uma janela natural para estudar a interação gravitacional; em particular, entender o estado final do colapso gravitacional e a formação de singularidades é um dos problemas fundamentais da física moderna. Nesta tese, iremos estudar vários modelos para objetos compactos e fluidos de matéria em colapso gravitacional no contexto de teorias afins da gravidade, em particular, iremos analisar como a inclusão de torsão no espaço-tempo afeta a estrutura e a dinâmica de objetos compactos massivos e a formação de singularidades. Na primeira parte, iremos desenvolver as ferramentas matemáticas que serão utilizadas ao longo da tese. Começamos por generalizar a decomposição covariante 1+3 para teorias afins da gravitação em espaços-tempo dotados de uma conexão afim, compatível com a métrica. Estes resultados mostram claramente como o tensor de torsão afeta a geometria dos espaços-tempo, em particular conclui-se que este influencia diretamente as quantidades cinemáticas de uma congruência, resolvendo muitos dos equívocos presentes na literatura. Investigamos as condições para o mergulho de uma variedade num espaço-tempo de maior dimensão, generalizando as equações de Gauss-Codazzi-Ricci para conexões afins compatíveis com a métrica. De seguida, estudamos a junção suave de dois espaços-tempo numa fronteira comum na presença de torsão, corrigindo e estendendo os resultados na literatura. A segunda parte desta tese é dedicada a singularidades do espaço-tempo. Expandimos o âmbito do teorema de Raychaudhuri-Komar na teoria da Relatividade Geral a uma larga gama de teorias da gravitação e mostramos como a presença de torsão e aceleração influencia a formação de singularidades. De seguida, consideramos o colapso de um fluido num espaço-tempo de Szekeres no contexto da teoria de Einstein-Cartan-Sciama-Kibble, encontrando um conjunto de condições aos dados iniciais para evitar a formação de singularidades. Na última parte consideramos soluções exatas para objetos compactos. Ao generalizar as equações de Tolman-Oppenheimer-Volkoff no contexto da teoria de Einstein-Cartan-Sciama-Kibble, derivamos e estudamos as propriedades de soluções exatas para objetos compactos permeados por um fluido perfeito composto por fermiões, suavemente combinados a um vácuo exterior. Também, provamos sob condições gerais que, no contexto de uma torsão do tipo de Weyssenhoff, não existem objetos compactos estáticos, esfericamente simétricos suportados apenas pelo momento angular intrínseco da matéria. Por fim, consideramos a junção dos espaços-tempo Minkowski — Reissner-Nordström com a presença de uma camada fina de matéria. Encontramos todas as soluções e investigamos as propriedades dos espaços-tempo resultantes.
The nature and evolution of massive astrophysical bodies provide a natural window to study the gravitational interaction; in particular, understanding the end state of gravitational collapse and the formation of singularities is one of the fundamental problems in modern physics. In this thesis, we will study several models for compact objects and matter fluids undergoing gravitational collapse in the context of affine theories of gravity, in particular, we will analyze how the inclusion of space-time torsion affects the structure and the dynamics of compact objects and the formation of singularities. In the first part, we develop a set of mathematical tools that will be used throughout the thesis. We start by generalizing the 1+3 covariant decomposition for generic affine theories of gravitation in space-times endowed with a metric compatible affine connection. These results, clearly show how the torsion tensor affects the geometry of the space-time, in particular it is found that it directly impacts the kinematical quantities of a congruence, solving many of the ambiguities lingering in the literature. We investigate the conditions for the embedding of a manifold in a higher dimensional space-time, generalizing the Gauss-Codazzi-Ricci equations for metric compatible affine connections. Then, we study the smooth matching of two space-times at a common boundary in the presence of torsion, correcting and extending the results in the literature. The second part of this thesis is devoted to space-time singularities. We extend the scope of the Raychaudhuri-Komar theorem of General Relativity to a wide class of theories of gravitation and show how the presence of torsion and acceleration influences the formation of singularities. We then consider the case of a collapsing fluid permeating a Szekeres space-time in the context of the Einstein-Cartan-Sciama-Kibble theory, finding a set of conditions on the initial data for the avoidance of singularities. In the last part we consider exact solutions for compact objects. Generalizing the Tolman-Oppenheimer-Volkoff equations in the context of the Einstein-Cartan-Sciama-Kibble theory, we derive and study the properties of exact solutions for compact objects permeated by a perfect fluid composed of fermions, smoothly matched to an exterior vacuum. Moreover, we prove under generic conditions that, in the context of a Weyssenhoff-like torsion, no static, spherically symmetric compact objects supported only by the intrinsic spin of matter can exist. Lastly, we consider the junction of a Minkwoski — Reissner-Nordström space-times by means of a thin matter shell. We find all the possible solutions and investigate the properties of the resulting space-times.
Supported by FCT-Portugal through Grant No. PD/BD/114074/2015, awarded in the framework of the Doctoral Programme IDPASC-Portugal.

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Bauswein, Andreas Ottmar [Verfasser]. „Relativistic simulations of compact object mergers for nucleonic matter and strange quark matter / Andreas Ottmar Bauswein“. 2010. http://d-nb.info/1000773221/34.

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Bücher zum Thema "Relativistic compact objects"

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Zdziarski, Andrzej A., und Marek Sikora, Hrsg. Relativistic Hadrons in Cosmic Compact Objects. Berlin, Heidelberg: Springer Berlin Heidelberg, 1991. http://dx.doi.org/10.1007/3-540-54789-4.

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Colpi, Monica, Piergiorgio Casella, Vittorio Gorini, Ugo Moschella und Andrea Possenti, Hrsg. Physics of Relativistic Objects in Compact Binaries: From Birth to Coalescence. Dordrecht: Springer Netherlands, 2009. http://dx.doi.org/10.1007/978-1-4020-9264-0.

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Physics of relativistic objects in compact binaries: From birth to coalescence. Dordrecht: Springer, 2009.

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1954-, Zdziarski Andrzej A., und Sikora Marek, Hrsg. Relativistic hadrons in cosmic compact objects: Proceedings of a workshop held in Koninki/Suhora, Poland, 9-11 October 1990. Berlin: Springer-Verlag, 1991.

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Zdziarski, Andrzej A. Relativistic Hadrons in Cosmic Compact Objects: Proceedings (Lecture Notes in Physics). Springer, 1992.

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Casella, Piergiorgio, Andrea Possenti, Monica Colpi, Vittorio Gorini und Ugo Moschella. Physics of Relativistic Objects in Compact Binaries: From Birth to Coalescence. Springer Netherlands, 2014.

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Sikora, Marek, und Andrzej A. Zdziarski. Relativistic Hadrons in Cosmic Compact Objects: Proceedings of a Workshop Held in Koninki/Suhora, Poland 9-11 October 1990. Springer, 2014.

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8

(Editor), Heon-Young Chang, Chang-Hwan Lee (Editor), Mannque Rho (Editor) und Insu Yi (Editor), Hrsg. Explosive Phenomena in Astrophysical Compact Objects: First KIAS Astrophysics Workshop, Seoul, Korea, 24-27 May 2000 (AIP Conference Proceedings / Astronomy and Astrophysics). American Institute of Physics, 2001.

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Zdziarski, Andrzej A. Relativistic Hadrons in Cosmic Compact Objects: Proceedings of a Workshop Held in Koninki/Suhora, Poland, 9-11 October 1990 (Lecture Notes in Physics). Springer, 1991.

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Buchteile zum Thema "Relativistic compact objects"

1

Perucho, M., und J. M. Martí. „Physical Parameters in Relativistic Jets from Compact Symmetric Objects“. In Highlights of Spanish Astrophysics II, 61–64. Dordrecht: Springer Netherlands, 2001. http://dx.doi.org/10.1007/978-94-017-1776-2_14.

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D'Amico, Nichi, und Marta Burgay. „Perspective in the Search for Relativistic Pulsars“. In Physics of Relativistic Objects in Compact Binaries: From Birth to Coalescence, 77–123. Dordrecht: Springer Netherlands, 2009. http://dx.doi.org/10.1007/978-1-4020-9264-0_3.

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Heuvel, E. P. J. van den. „The Formation and Evolution of Relativistic Binaries“. In Physics of Relativistic Objects in Compact Binaries: From Birth to Coalescence, 125–98. Dordrecht: Springer Netherlands, 2009. http://dx.doi.org/10.1007/978-1-4020-9264-0_4.

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Stella, L. „Strong Gravitational Field Diagnostics in Binary Systems Containing a Compact Object“. In Physics of Relativistic Objects in Compact Binaries: From Birth to Coalescence, 265–80. Dordrecht: Springer Netherlands, 2009. http://dx.doi.org/10.1007/978-1-4020-9264-0_7.

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Damour, Thibault. „Binary Systems as Test-Beds of Gravity Theories“. In Physics of Relativistic Objects in Compact Binaries: From Birth to Coalescence, 1–41. Dordrecht: Springer Netherlands, 2009. http://dx.doi.org/10.1007/978-1-4020-9264-0_1.

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Kramer, Michael. „Exploiting Binary Pulsars as Laboratories of Gravity Theories“. In Physics of Relativistic Objects in Compact Binaries: From Birth to Coalescence, 43–75. Dordrecht: Springer Netherlands, 2009. http://dx.doi.org/10.1007/978-1-4020-9264-0_2.

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Colpi, Monica, und Bernadetta Devecchi. „Dynamical Formation and Evolution of Neutron Star and Black Hole Binaries in Globular Clusters“. In Physics of Relativistic Objects in Compact Binaries: From Birth to Coalescence, 199–243. Dordrecht: Springer Netherlands, 2009. http://dx.doi.org/10.1007/978-1-4020-9264-0_5.

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Lazzati, Davide, und Rosalba Perna. „Short Gamma Ray Bursts: Marking the Birth of Black Holes from Coalescing Compact Binaries“. In Physics of Relativistic Objects in Compact Binaries: From Birth to Coalescence, 245–63. Dordrecht: Springer Netherlands, 2009. http://dx.doi.org/10.1007/978-1-4020-9264-0_6.

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Israel, Gian Luca, und Simone Dall'Osso. „White Dwarfs in Ultrashort Binary Systems“. In Physics of Relativistic Objects in Compact Binaries: From Birth to Coalescence, 281–304. Dordrecht: Springer Netherlands, 2009. http://dx.doi.org/10.1007/978-1-4020-9264-0_8.

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Pretorius, Frans. „Binary Black Hole Coalescence“. In Physics of Relativistic Objects in Compact Binaries: From Birth to Coalescence, 305–69. Dordrecht: Springer Netherlands, 2009. http://dx.doi.org/10.1007/978-1-4020-9264-0_9.

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Konferenzberichte zum Thema "Relativistic compact objects"

1

Wu, Kinwah, Steven V. Fuerst, Ye-Fei Yuan, Xiang-Dong Li und Dong Lai. „General Relativistic Radiative Transfer“. In ASTROPHYSICS OF COMPACT OBJECTS: International Conference on Astrophysics of Compact Objects. AIP, 2008. http://dx.doi.org/10.1063/1.2840444.

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van Adelsberg, Matthew, Davide Lazzati, Rosalba Perna, Ye-Fei Yuan, Xiang-Dong Li und Dong Lai. „Ultra-Relativistic Shockwaves in Arbitrary Continuous Media I“. In ASTROPHYSICS OF COMPACT OBJECTS: International Conference on Astrophysics of Compact Objects. AIP, 2008. http://dx.doi.org/10.1063/1.2840431.

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Chatterjee, Sujit. „Large redshifts from compact objects“. In RELATIVISTIC ASTROPHYSICS: 20th Texas Symposium. AIP, 2001. http://dx.doi.org/10.1063/1.1419607.

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McKinney, Jonathan C. „General Relativistic Magnetohydrodynamical Models of Relativistic Jets“. In THE MULTICOLORED LANDSCAPE OF COMPACT OBJECTS AND THEIR EXPLOSIVE ORIGINS. American Institute of Physics, 2007. http://dx.doi.org/10.1063/1.2774844.

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Spruit, Hendrik. „Relativistic jet production from accreting compact objects“. In VI Microquasar Workshop: Microquasars and Beyond. Trieste, Italy: Sissa Medialab, 2007. http://dx.doi.org/10.22323/1.033.0044.

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Tchekhovskoy, Alexander, Jonathan C. McKinney, Ramesh Narayan und Magnus Axelsson. „Force-free Simulations of Ultra-Relativistic Jets“. In COOL DISCS, HOT FLOWS: The Varying Faces of Accreting Compact Objects. AIP, 2008. http://dx.doi.org/10.1063/1.3002510.

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Pelletier, G., Martin Lemoine und Illya Plotnikov. „Relativistic outflows from compact objects and generation of Astroparticles“. In Frontiers of Fundamental Physics 14. Trieste, Italy: Sissa Medialab, 2016. http://dx.doi.org/10.22323/1.224.0033.

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Bakala, Pavel, Eva Šrámková, Zdeněk Stuchlík, Gabriel Török und Magnus Axelsson. „On magnetic-field induced non-geodesic corrections to the relativistic precession QPO model“. In COOL DISCS, HOT FLOWS: The Varying Faces of Accreting Compact Objects. AIP, 2008. http://dx.doi.org/10.1063/1.3002494.

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Jiménez‐Bailón, E., E. Piconcelli, M. Sánchez‐Portal, G. Matt, M. Guainazzi, A. Martocchia, M. Motch, A. Schroder und S. Bianchi. „XMM‐Newton view of the relativistic Fe Kα feature in the intermediate Seyfert galaxy 4U 1344‐60“. In THE MULTICOLORED LANDSCAPE OF COMPACT OBJECTS AND THEIR EXPLOSIVE ORIGINS. American Institute of Physics, 2007. http://dx.doi.org/10.1063/1.2774943.

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Shaghaghian, Mahboobeh. „Accreting Magnetofluids around a Rotating Compact Object with a Dipolar Magnetic Field“. In 25th Texas Symposium on Relativistic Astrophysics. Trieste, Italy: Sissa Medialab, 2011. http://dx.doi.org/10.22323/1.123.0019.

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