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Telescopes --- Black holes (Astronomy) --- Outer space --- Exploration.
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Que sait-on des trous noirs ? Peut-on les observer ? Qu'y a-t-il à l'intérieur ? Existent-ils vraiment ?Les trous noirs sont des astres fascinants, des sphères dans l'espace dont rien ne peut s'échapper. De tels objets ne peuvent ni émettre, ni réfléchir la lumière, mais certains sont pourtant extraordinairement lumineux. Toutefois, ce n'est pas là leur seule bizarrerie : dans un trou noir, l'espace se change en temps, le temps en espace, et nul ne connaît la véritable nature de la singularité centrale.
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Albert Einstein's General Theory of Relativity, published in 1915, made a remarkable prediction: gravitational radiation. Just like light (electromagnetic radiation), gravity could travel through space as a wave and affect any objects it encounters by alternately compressing and expanding them. However, there was a problem. The force of gravity is around a trillion, trillion, trillion times weaker than electromagnetism so the calculated compressions and expansions were incredibly small, even for gravity waves resulting from a catastrophic astrophysical event such as a supernova explosion in our own galaxy. Discouraged by this result, physicists and astronomers didn't even try to detect these tiny, tiny effects for over 50 years. Then, in the late 1960s and early 1970s, two events occurred which started the hunt for gravity waves in earnest. The first was a report of direct detection of gravity waves thousands of times stronger than even the most optimistic calculation. Though ultimately proved wrong, this result started scientists thinking about what instrumentation might be necessary to detect these waves. The second was an actual, though indirect, detection of gravitational radiation due to the effects it had on the period of rotation of two 'neutron stars' orbiting each other. In this case, the observations were in exact accord with predictions from Einstein's theory, which confirmed that a direct search might ultimately be successful. Nevertheless, it took another 40 years of development of successively more sensitive detectors before the first real direct effects were observed in 2015, 100 years after gravitational waves were first predicted. This is the story of that hunt, and the insight it is producing into an array of topics in modern science, from the creation of the chemical elements to insights into the properties of gravity itself.
Gravitational waves. --- Black holes (Astronomy) --- Neutron stars. --- Astrophysics. --- SCIENCE / Physics / Astrophysics.
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The formation of the first supermassive black holes is one of the main open questions in our understanding of high-redshift structure formation. In this book, we aim to provide a summary of state-of-the-art modern research on this topic, exploring the formation of massive black holes from a fluid-dynamical, stellar-dynamical and chemical perspective. The book thus presents a solid theoretical foundation, a comparison with current observations and future observational perspectives with upcoming missions such as the Square Kilometre Array, the European Extremely Large Telescope, the Euclid satellite as well as possible detections via gravitational waves.
Black holes (Astronomy) --- Red shift. --- Astrophysics. --- Trous noirs (astronomie) --- Décalage vers le rouge. --- Astrophysique.
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Galaxies --- Black holes (Astronomy) --- Magnetic fields. --- Observations. --- Chandra X-ray Observatory (U.S.) --- Event Horizon Telescope. --- M87 (Galaxy)
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The ultimate proofs that black holes exist have been obtained very recently thanks to the detection of gravitational waves from their coalescence and due to material orbiting at a distance of some gravitational radii imaged by optical interferometry or X-ray reverberation mapping. This book provides three comprehensive and up-to-date reviews covering the gravitational wave breakthrough, our understanding of accretion and feedback in supermassive black holes and the relevance of black holes for the Universe since the Big Bang. Neil J. Cornish presents gravitational wave emission from black hole mergers and the physics of detection. Andrew King reviews the physics of accretion on to supermassive black holes and their feedback on host galaxies. Tiziana Di Matteo addresses our understanding of black hole formation at cosmic dawn, the emergence of the first quasars, black hole merging and structure formation. The topics covered by the 48th Saas-Fee Course provide a broad overview of the importance of black holes in modern astrophysics.
Black holes (Astronomy) --- Frozen stars --- Compact objects (Astronomy) --- Gravitational collapse --- Stars --- Astrophysics. --- Cosmology. --- Astrophysics and Astroparticles. --- Astronomy --- Deism --- Metaphysics --- Astronomical physics --- Cosmic physics --- Physics
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During the past few decades, plasma science has witnessed a great growth in laboratory studies, in simulations, and in space. Plasma is the most common phase of ordinary matter in the universe. It is a state in which ionized matter (even as low as 1%) becomes highly electrically conductive. As such, long-range electric and magnetic fields dominate its behavior. Cosmic plasmas are mostly associated with stars, supernovae, pulsars and neutron stars, quasars and active galaxies at the vicinities of black holes (i.e., their jets and accretion disks). Cosmic plasma phenomena can be studied with different methods, such as laboratory experiments, astrophysical observations, and theoretical/computational approaches (i.e., MHD, particle-in-cell simulations, etc.). They exhibit a multitude of complex magnetohydrodynamic behaviors, acceleration, radiation, turbulence, and various instability phenomena. This Special Issue addresses the growing need of the plasma science principles in astrophysics and presents our current understanding of the physics of astrophysical plasmas, their electromagnetic behaviors and properties (e.g., shocks, waves, turbulence, instabilities, collimation, acceleration and radiation), both microscopically and macroscopically. This Special Issue provides a series of state-of-the-art reviews from international experts in the field of cosmic plasmas and electromagnetic phenomena using theoretical approaches, astrophysical observations, laboratory experiments, and state-of-the-art simulation studies.
cosmic ray knee and ankle --- blazars --- numerical methods --- global jets --- MHD–accretion --- muti-messenger astronomy --- massive star supernovae --- galaxies: active --- TBD --- 26Al --- black holes --- accreting black holes --- particle-in-cell simulations --- kink-like instability --- laser-induced nuclear reactions --- magnetic fields --- magneto-hydrodynamics --- gamma-ray bursts --- active galactic nuclei --- accretion discs–jets --- numerical relativity --- plasma physics --- GRMHD --- high-power laser systems --- radio interferometry --- recollimation shocks --- effective lifetime --- multi-wavelength astronomy --- relativistic jets --- high energy astrophysics --- jets --- active galaxies --- relativistic astrophysics --- helical magnetic fields --- laser plasma --- X-ray binaries --- polarization --- the Weibel instability --- AGN --- neutrino astrophysics --- radiation mechanism: non-thermal --- nuclear astrophysics --- cosmic rays --- mushroom instability --- accretion disks --- MHD winds
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Ce livre est une invitation à découvrir le lien profond qui unit la relativité générale (la théorie de la gravitation d'Einstein) et la géométrie différentielle, branche de la géométrie issue de la découverte des géométries non-euclidiennes par Gauss et Riemann au XIXe siècle. En abordant la relativité par ses aspects géométriques, ce livre montre que les phénomènes surprenants de la relativité, tels que le paradoxe des jumeaux, les boucles temporelles, les trous noirs, les trous de ver, ne sont que des conséquences de la géométrie de l'espace-temps. Le livre explore également la fascinante relation entre les mathématiques et la physique à travers une des théories les plus passionnantes de notre siècle, la relativité générale, sujet particulièrement d'actualité depuis les récentes observations des ondes gravitationnelles et les observations de plus en plus directes des trous noirs. Il montre ainsi que les mathématiques, loin d'être simplement un « outil », sont une des sources d'inspiration les plus fécondes des physiciens théoriciens. Ce livre offrira une introduction plaisante aux mathématiques de la relativité, autant à l'étudiant en sciences qu'au lecteur curieux et motivé par les découvertes scientifiques les plus fascinantes de notre époque.
Black holes (Astronomy) --- Mathematical physics. --- Relativity (Physics) --- Physical mathematics --- Physics --- Gravitation --- Nonrelativistic quantum mechanics --- Space and time --- Frozen stars --- Compact objects (Astronomy) --- Gravitational collapse --- Stars --- Mathematics --- Geometry, Differential. --- Cosmology. --- Relativité (physique) --- Géométrie différentielle. --- Trous noirs (astronomie) --- Physique mathématique. --- Cosmologie. --- Relativité (physique) --- Géométrie différentielle. --- Physique mathématique.
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Notre Univers a-t-il un début ? Est-il unique ?La science moderne a révolutionné notre compréhension de l'Univers. Il est maintenant possible de connaître certains aspects des processus qui eurent lieu moins d'un milliardième de milliardième de milliardième de seconde après le Big Bang.Dans cette nouvelle édition actualisée, Aurélien Barrau décrit le cosmos qui se dessine sous nos yeux. Trous noirs, modèle standard de la physique des particules, gravité... les piliers et les énigmes du Big Bang sont abordés les uns après les autres, à la manière d'une balade aux origines de l'Univers.
Big bang theory --- Expanding universe --- Relativistic astrophysics --- Black holes (Astronomy) --- Quantum cosmology --- Cosmic background radiation --- Gravitational waves --- Quantum gravity --- String models --- Big bang --- Univers --- Astrophysique relativiste --- Trous noirs (astronomie) --- Cosmologie quantique --- Rayonnement du fond du ciel --- Rayonnement gravitationnel --- Gravité quantique. --- Modèles des cordes vibrantes (physique nucléaire) --- Expansion --- Big bang theory. --- Expanding universe. --- Relativistic astrophysics. --- Quantum cosmology. --- Cosmic background radiation. --- Gravitational waves. --- Quantum gravity. --- String models. --- Big bang. --- Astrophysique relativiste. --- Cosmologie quantique. --- Rayonnement du fond du ciel. --- Ondes gravitationnelles. --- Théorie des cordes. --- Expansion. --- Gravité quantique. --- Théorie des cordes.
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Based on Prof. Lüst's Masters course at the University of Munich, this book begins with a short introduction to general relativity. It then presents black hole solutions, and discusses Penrose diagrams, black hole thermodynamics and entropy, the Unruh effect, Hawking radiation, the black hole information problem, black holes in supergravity and string theory, the black hole microstate counting in string theory, asymptotic symmetries in general relativity, and a particular quantum model for black holes. The book offers an up-to-date summary of all the pertinent questions in this highly active field of physics, and is ideal reading for graduate students and young researchers.
Black holes (Astronomy) --- Thermodynamics. --- Classical and Quantum Gravitation, Relativity Theory. --- Cosmology. --- Quantum Field Theories, String Theory. --- Chemistry, Physical and theoretical --- Dynamics --- Mechanics --- Physics --- Heat --- Heat-engines --- Quantum theory --- Gravitation. --- Quantum field theory. --- String theory. --- Models, String --- String theory --- Nuclear reactions --- Relativistic quantum field theory --- Field theory (Physics) --- Relativity (Physics) --- Astronomy --- Deism --- Metaphysics --- Matter --- Antigravity --- Centrifugal force --- Properties --- Forats negres (Astronomia) --- Cosmologia --- Termodinàmica --- Termologia --- Dinàmica --- Física --- Mecànica --- Bombes de calor --- Dinàmica de gasos --- Entalpia --- Entropia --- Mecànica estadística --- Processos irreversibles --- Radiació del cos negre --- Segon principi de la termodinàmica --- Termodinàmica atmosfèrica --- Termodinàmica del desequilibri --- Termoelasticitat --- Termoquímica --- Transferència de massa --- Anàlisi tèrmica --- Calor --- Fred --- Màquines tèrmiques --- Motors tèrmics --- Teoria quàntica --- Univers (Metafísica) --- Deisme --- Filosofia de la natura --- Metafísica --- Antropocentrisme --- Big Bang --- Cosmologia islàmica --- Cosmologia jueva --- Cosmologia quàntica --- Etern retorn --- Expansió de l'univers --- Hipòtesi nebular --- Macrocosmos --- Microcosmos --- Monadologia --- Origen del sistema solar --- Origen dels planetes --- Pluralitat de mons --- Principi antròpic --- Quatre elements (Filosofia) --- Teleologia --- Teosofia --- Creació --- Col·lapse gravitacional --- String models.
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