LEADER 04718nam 22007575 450 001 9910254638503321 005 20200705080211.0 010 $a1-4939-3550-X 024 7 $a10.1007/978-1-4939-3550-5 035 $a(CKB)3710000000579431 035 $a(EBL)4386718 035 $a(SSID)ssj0001607095 035 $a(PQKBManifestationID)16316772 035 $a(PQKBTitleCode)TC0001607095 035 $a(PQKBWorkID)14895984 035 $a(PQKB)11142710 035 $a(DE-He213)978-1-4939-3550-5 035 $a(MiAaPQ)EBC4386718 035 $a(PPN)191705985 035 $a(EXLCZ)993710000000579431 100 $a20160129d2016 u| 0 101 0 $aeng 135 $aur|n|---||||| 181 $ctxt 182 $cc 183 $acr 200 14$aThe Strongest Magnetic Fields in the Universe /$fedited by Vasily S. Beskin, A. Balogh, Maurizio Falanga, Maxim Lyutikov, Sandro Mereghetti, Tsvi Piran, R.A. Treumann 205 $a1st ed. 2016. 210 1$aNew York, NY :$cSpringer New York :$cImprint: Springer,$d2016. 215 $a1 online resource (579 p.) 225 1 $aSpace Sciences Series of ISSI,$x1385-7525 ;$v54 300 $a"Previously published in Space Science Reviews Volume 191, Issues 1- 4, 2015." 311 $a1-4939-3549-6 320 $aIncludes bibliographical references. 327 $aForeword -- Part I: Introduction -- Magnetic Fields at Largest Universal Strengths: Overview -- Physics in Very Strong Magnetic Fields: An Introduction -- Part II: Magnetic Fields in Stars -- Observations of Strong Magnetic Fields in Nondegenerate Stars -- Magnetic Field Generation in Stars -- Magnetic White Dwarfs -- Part III: Neutron Stars -- Neutron Stars: Thermal Emitters -- Radio Pulsars -- Neutron Stars: Cooling and Transport -- Magnetic Fields of Neutron Stars in X-ray Binaries -- Magnetars: Properties, Origin and Evolution -- Part IV: Accretion, Winds, Jets -- Accretion and Outflows from Magnetized Stars -- Pulsar Wind Nebulae -- Disks and Jets: Gravity, Rotation and Magnetic Fields -- Part V: Physical Processes -- Gamma Ray Bursts As Sources of Strong Magnetic Fields -- Relativistic Shocks Particle Acceleration and Magnetization -- Relativistic Magnetic Reconnection and Its Astrophysical Applications. 330 $aThis volume extends the ISSI series on magnetic fields in the Universe into the domain of what are by far the strongest fields in the Universe, and stronger than any field that could be produced on Earth. The chapters describe the magnetic fields in non-degenerate strongly magnetized stars, degenerate stars (such as white dwarfs and neutron stars), exotic members called magnetars, and in their environments, as well as magnetic fields in the environments of black holes. These strong fields have a profound effect on the behavior of matter, visible in particular in highly variable processes like radiation in all known wavelengths, including Gamma-Ray bursts. The generation and structure of such strong magnetic fields and effects on the environment are also described. 410 0$aSpace Sciences Series of ISSI,$x1385-7525 ;$v54 606 $aSpace sciences 606 $aCosmology 606 $aMagnetism 606 $aMagnetic materials 606 $aSpace Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics)$3https://scigraph.springernature.com/ontologies/product-market-codes/P22030 606 $aCosmology$3https://scigraph.springernature.com/ontologies/product-market-codes/P22049 606 $aMagnetism, Magnetic Materials$3https://scigraph.springernature.com/ontologies/product-market-codes/P25129 615 0$aSpace sciences. 615 0$aCosmology. 615 0$aMagnetism. 615 0$aMagnetic materials. 615 14$aSpace Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics). 615 24$aCosmology. 615 24$aMagnetism, Magnetic Materials. 676 $a523.0188 702 $aBeskin$b Vasily S$4edt$4http://id.loc.gov/vocabulary/relators/edt 702 $aBalogh$b A$4edt$4http://id.loc.gov/vocabulary/relators/edt 702 $aFalanga$b Maurizio$4edt$4http://id.loc.gov/vocabulary/relators/edt 702 $aLyutikov$b Maxim$4edt$4http://id.loc.gov/vocabulary/relators/edt 702 $aMereghetti$b Sandro$4edt$4http://id.loc.gov/vocabulary/relators/edt 702 $aPiran$b Tsvi$4edt$4http://id.loc.gov/vocabulary/relators/edt 702 $aTreumann$b R.A$4edt$4http://id.loc.gov/vocabulary/relators/edt 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910254638503321 996 $aStrongest Magnetic Fields in the Universe$91821442 997 $aUNINA