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Selected Papers from 43rd International Conference of Theoretical Physics: Matter to the Deepest, Recent Developments In Physics Of Fundamental Interactions (MTTD2019)

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ISBN: 9783039283705 9783039283712 Year: Pages: 94 DOI: 10.3390/books978-3-03928-371-2 Language: English
Publisher: MDPI - Multidisciplinary Digital Publishing Institute
Subject: Science (General) --- Physics (General)
Added to DOAB on : 2020-04-07 23:07:09
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Understanding the origins of the Universe and how it works and evolves is the present mission of a large community of physicists. It calls for a large scale vision, involving general relativity, astrophysics, and cosmology. Theoretical physics is presently at an important moment in its history. As predicted by Einstein, gravitational waves have been experimentally proven to exist. With the discovery of the Higgs boson, the set of interactions and elementary particles that is called the ""standard model"" (SM), is complete. Yet the Higgs boson itself, and how it breaks the electroweak symmetry, remains a fascinating subject requiring further studies and verification. Furthermore, several experimental facts are not accounted for by the SM: (i) the baryon asymmetry of the Universe, (ii) the nature and origin of dark matter, and (iii) the origin of neutrino masses; these have no unique, if any, explanation in the SM and yet will require answers from particle physics. We need to explore further both SM and its extensions. This is a subject of papers included in this book, which gives representation to the topics discussed during the Matter to the Deepest conference in 2019 in Poland (http://indico.if.us.edu.pl/event/5).

Compact Stars in the QCD Phase Diagram

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ISBN: 9783039219582 9783039219599 Year: Pages: 273 DOI: 10.3390/books978-3-03921-959-9 Language: English
Publisher: MDPI - Multidisciplinary Digital Publishing Institute
Subject: Science (General) --- Mathematics
Added to DOAB on : 2020-01-30 16:39:46
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The book edition of the Universe Special Issue “Compact Stars in the QCD Phase Diagram” is devoted to the overarching aspects shared between heavy-ion collisions and compact star astrophysics in investigating the hadron-to-quark matter phase transition in the equation of state of strongly interacting matter in different regions of the phase diagram of QCD. It comprises 22 review and research articles that, together, will serve as a useful guide in educating both young and senior scientists in this emerging field that represents an intersection of the communities of strongly interacting matter theory, heavy-ion collision physics and compact star astrophysics.

Keywords

heavy-ion collisions --- directed flow --- hydrodynamics --- deconfinement --- hybrid stars --- neutron stars --- equation of state --- ? meson condensation --- maximum mass --- ? resonances --- finite temperature --- finite density --- quark-gluon plasma --- finite size --- speed of sound --- neutron stars --- equation of state --- in-medium effects --- neutrino --- Quantum Chromodynamics --- dense matter --- vector interaction --- neutron stars --- equation of state --- QCD matter --- phase transition --- critical point --- modified excluded-volume mechanism --- dense matter --- equation of state --- stars: neutron --- pulsars: general, pulsars: PSR J0737 ? 3039A --- pulsars: PSR J1757 ? 1854 --- relativistic heavy-ion collisions --- monte carlo simulations --- transport theory --- strangeness --- neutron stars --- star oscillations --- hadron–quark continuity --- neutron stars --- QCD phase diagram --- neutron stars --- stellar magnetic field --- stellar structure --- stellar evolution --- neutron star --- equation of state --- phase transition --- quark matter --- pulsars --- quark stars --- general relativity --- Gravitational waves --- Gamma-ray bursts --- nuclear matter --- neutron stars --- quarks --- combustion --- neutron star --- QCD matter --- phase transition --- critical point --- neutron stars --- gravitational waves --- equation of state --- chiral symmetry --- axion QED --- quark-hole pairing --- cold-dense QCD --- magnetic DCDW --- quark matter --- hadronic matter --- quark deconfinement --- neutron star matter --- nuclear equation of state --- phase transition --- crystalline structure --- neutrino emissivities --- cluster virial expansion --- quark-hadron matter --- Mott dissociation --- Beth-Uhlenbeck equation of state --- heavy-ion collisions --- supernova explosions --- mass-twin stars --- nuclear symmetry energy --- heavy-ion collisions --- transport theory --- collective flow --- light cluster emission --- meson production --- quark-hadron phase transition --- pasta phases --- speed of sound --- hybrid compact stars --- mass-radius relation --- GW170817

Cosmic Plasmas and Electromagnetic Phenomena

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ISBN: 9783039214655 9783039214662 Year: Pages: 264 DOI: 10.3390/books978-3-03921-466-2 Language: English
Publisher: MDPI - Multidisciplinary Digital Publishing Institute
Subject: Science (General) --- Physics (General) --- Astronomy (General)
Added to DOAB on : 2019-12-09 11:49:16
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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.

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