LEADER 03906nam  22006375  450 
001 9910552719703321
005 20251113182210.0
010   $a3-030-85198-2
024 7 $a10.1007/978-3-030-85198-9
035   $a(MiAaPQ)EBC6926779
035   $a(Au-PeEL)EBL6926779
035   $a(CKB)21403602500041
035   $a(PPN)261518356
035   $a(OCoLC)1304247995
035   $a(DE-He213)978-3-030-85198-9
035   $a(EXLCZ)9921403602500041
100   $a20220315d2022      u|         0
101 0 $aeng
135   $aurcnu||||||||
181   $ctxt$2rdacontent
182   $cc$2rdamedia
183   $acr$2rdacarrier
200 10$aMillisecond Pulsars /$fedited by Sudip Bhattacharyya, Alessandro Papitto, Dipankar Bhattacharya
205   $a1st ed. 2022.
210  1$aCham :$cSpringer International Publishing :$cImprint: Springer,$d2022.
215   $a1 online resource (334 pages)
225 1 $aAstrophysics and Space Science Library,$x2214-7985 ;$v465
311 08$aPrint version: Bhattacharyya, Sudip Millisecond Pulsars Cham : Springer International Publishing AG,c2022 9783030851972 
320   $aIncludes bibliographical references and index.
327   $aChapter 1: Radio Millisecond Pulsars -- Chapter 2: The High-Energy Emission of Millisecond Pulsars -- Chapter 3: The Emission Physics of Millisecond Pulsars -- Chapter 4: Accretion Powered X-ray Millisecond Pulsars -- Chapter 5: Nuclear-powered X-ray millisecond pulsars -- Chapter 6: Transitional millisecond pulsars -- Chapter 7: Origin and Binary Evolution of Millisecond Pulsars -- Chapter 8: Millisecond Magnetars -- Chapter 9: The Equation of State of Neutron Star Matter. Index.
330   $aThis book includes nine chapters written by internationally recognized experts, covering all aspects of millisecond pulsars in one concise and cohesive volume. These aspects include pulsations powered by stellar spin, accretion and thermonuclear burning of accreted matter, their physics and utility, stellar evolution and the extreme physics of super-dense stellar cores. The book includes substantial background material as well as recent theoretical and multi-wavelength observational results. The volume will thus be useful for professional astronomers and graduate students alike. What is the behavior of the strong nuclear interaction, and what are the matter constituents at ultrahigh densities in neutron star cores? How do old neutron stars in binaries evolve? How does their magnetosphere interact with the surrounding plasma to accelerate particles and emit radiation observed at all wavelengths? These are just a few of the questions that millisecond pulsarsare helping us answer and will settle in the near future with the next generation of instruments. Such quickly rotating, highly magnetized neutron stars are remarkable natural laboratories that allow us to investigate the fundamental constituents of matter and their interactions under extreme conditions that cannot be reproduced in terrestrial laboratories.
410  0$aAstrophysics and Space Science Library,$x2214-7985 ;$v465
606   $aAstrophysics
606   $aAstronomy$vObservations
606   $aAstronomy
606   $aAstrophysics
606   $aAstronomy, Observations and Techniques
606   $aAstronomy, Cosmology and Space Sciences
615  0$aAstrophysics.
615  0$aAstronomy
615  0$aAstronomy.
615 14$aAstrophysics.
615 24$aAstronomy, Observations and Techniques.
615 24$aAstronomy, Cosmology and Space Sciences.
676   $a523.8874
676   $a523.8874
702   $aBhattacharyya$b Sudip
702   $aPapitto$b Alessandro
702   $aBhattacharya$b Dipankar$c(Astrophysicist)
801  0$bMiAaPQ
801  1$bMiAaPQ
801  2$bMiAaPQ
906   $aBOOK
912   $a9910552719703321
996   $aMillisecond pulsars$92960524
997   $aUNINA