Nicht aus der Schweiz? Besuchen Sie lehmanns.de
Für diesen Artikel ist leider kein Bild verfügbar.

The First Stars

(Autor)

Buch | Hardcover
X, 240 Seiten
2025 | 1st ed. 2024
Springer Berlin (Verlag)
978-3-642-11964-4 (ISBN)
CHF 104,75 inkl. MwSt
  • Noch nicht erschienen - erscheint am 13.06.2025
  • Versandkostenfrei
  • Auch auf Rechnung
  • Artikel merken

This book is based in part on classroom tested lectures related to the first stars (Pop III stars), but also draws from the author's review articles of the main physical principles involved. The book will thus combine pedagogical introductory chapters with more advanced ones to survey the cutting-edge advances from the frontier of research.

The formation of Pop III stars and galaxies is one of the great outstanding challenges in modern astrophysics and cosmology. The first stars are likely key drivers for early cosmic evolution and will be at the center of attention over the next decade. The best available space and ground-based telescopes like the Hubble Space Telescope probe the Universe to high redshifts and provide us with tantalizing hints; but they cannot yet directly detect the first generation of stars and the formation of the first galaxies. This is left as key science for future telescopes like the James Webb Space Telescope.

The book covers the theoryof first star formation, the relation between first stars and dark matter, their impact on cosmology, their observational signatures, the transition to normal star formation as well as the assembly of the first galaxies. It will prepare advanced students and researchers entering the field for interpreting observational findings and their cosmological implications.

Volker Bromm is a professor in the Department of Astronomy at the University of Texas at Austin. His research focuses on star and galaxy formation during the first billion years of cosmic history, employing supercomputer simulations and other approaches in theoretical astrophysics. Bromm's work has contributed to the emerging theoretical framework for early cosmological structure formation, making predictions for the next generation of observational facilities that will probe the first stars and galaxies in the coming decade.

Introduction: the first stars and galaxies as key drivers of early cosmic evolution; key science for the upcoming JWST.- The Cosmological Context: CDM cosmology; cooling in primordial gas; Rees-Ostriker criterion; prediction of minihalos as sites of first star formation.- Population III Star Formation: gravitational instability and initial collapse; protostellar accretion; feedback processes: the final stellar mass; binaries, multiples, clusters; neglected processes in the 'Standard Model' - magnetic fields, cosmic rays.- Dark Matter and the First Stars: warm dark matter: - implies different star formation sites - suppresses star formation rate; 'Dark Stars': DM heating - Pop III red supergiants.- Impact on cosmology: radiative feedback and the beginning of reionization; chemical feedback: the first supernova explosions.- Transition to normal star formation: physics of the 'Critical Metallicity'; turbulence and formation of star clusters.- Formation of the First Galaxies.- Observational signature: recombination line radiation; supernova searches with JWST; stellar archaeology; cosmic backgrounds: 21 cm radiation, infrared background.- Epilogue Introduction: the first stars and galaxies as key drivers of early cosmic evolution; key science for the upcoming JWST.- The Cosmological Context: CDM cosmology; cooling in primordial gas; Rees-Ostriker criterion; prediction of minihalos as sites of first star formation.- Population III Star Formation: gravitational instability and initial collapse; protostellar accretion; feedback processes: the final stellar mass; binaries, multiples, clusters; neglected processes in the 'Standard Model' - magnetic fields, cosmic rays.- Dark Matter and the First Stars: warm dark matter: - implies different star formation sites - suppresses star formation rate; 'Dark Stars': DM heating - Pop III red supergiants.- Impact on cosmology: radiative feedback and the beginning of reionization; chemical feedback: the first supernova explosions.- Transition to normal star formation: physics of the 'Critical Metallicity'; turbulence and formation of star clusters.- Formation of the First Galaxies.- Observational signature: recombination line radiation; supernova searches with JWST; stellar archaeology; cosmic backgrounds: 21 cm radiation, infrared background.- Epilogue.

Erscheint lt. Verlag 13.6.2025
Reihe/Serie Astronomy and Astrophysics Library
Zusatzinfo 240 p. 80 illus., 10 illus. in color.
Verlagsort Berlin
Sprache englisch
Maße 155 x 235 mm
Themenwelt Naturwissenschaften Physik / Astronomie Astronomie / Astrophysik
Naturwissenschaften Physik / Astronomie Atom- / Kern- / Molekularphysik
Schlagworte Dark Matter • Early Universe • first generation stars • First Stars textbook • Galaxy Formation • Hardcover, Softcover / Physik, Astronomie/Astronomie • Infrared Astronomy • JWST • Mini Halos • Pop III • Population III stars • Reionization • star formation • Stern (Astronomie)
ISBN-10 3-642-11964-6 / 3642119646
ISBN-13 978-3-642-11964-4 / 9783642119644
Zustand Neuware
Haben Sie eine Frage zum Produkt?
Mehr entdecken
aus dem Bereich
Der Wettstreit Dunkler Materie und Dunkler Energie: Ist das Universum …

von Adalbert W. A. Pauldrach; Tadziu Hoffmann

Buch | Hardcover (2022)
Springer (Verlag)
CHF 69,95
die Geschichte und Erforschung unserer Galaxie

von Harald Lesch; Cecilia Scorza-Lesch; Arndt Latußeck

Buch | Hardcover (2023)
C.Bertelsmann (Verlag)
CHF 40,80