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[null,"1.","Record Nr.",null,"UNINA9910454514703321"]
[null,null,"Autore",null,"Perkins Donald H"]
[null,null,"Titolo",null,"Particle astrophysics [[electronic resource] /] / D.H. Perkins"]
[null,null,"Pubbl/distr/stampa",null,"Oxford ; ; New York, : Oxford University Press, 2009"]
[null,null,"ISBN",null,"1-282-05333-7"]
[{"$nulls":4},"9786612053337"]
[{"$nulls":4},"0-19-156280-7"]
[null,null,"Edizione",null,"[2nd ed.]"]
[null,null,"Descrizione fisica",null,"1 online resource (356 p.)"]
[null,null,"Collana",null,"Oxford master series in physics ; ; 10"]
[{"$nulls":4},"Oxford master series in physics. Particle physics, astrophysics, and cosmology"]
[null,null,"Disciplina",null,"523.01/97"]
[null,null,"Soggetti",null,"Nuclear astrophysics"]
[{"$nulls":4},"Particles (Nuclear physics)"]
[{"$nulls":4},"Electronic books."]
[null,null,"Lingua di pubblicazione",null,"Inglese"]
[null,null,"Formato",null,"Materiale a stampa"]
[null,null,null,"Livello bibliografico","Monografia"]
[null,null,null,"Note generali","Description based upon print version of record."]
[null,null,null,"Nota di bibliografia","Includes bibliographical references (p. [329]-334) and index."]
[null,null,"Nota di contenuto",null,"Contents; Part 1 Particles and Interactions; Part 2 The Early Universe; Part 3 Particles and Radiation in the Cosmos; A: Table of physical constants; B: Yukawa theory and the boson propagator; C: Perturbative growth of structure in the early universe; D: The MSW mechanism in solar neutrino interactions; Answers to problems; References; Bibliography; Index"]
[null,null,null,"Sommario/riassunto","How did our universe begin? An understanding of the development of the early universe brings together the subjects of particle physics, astrophysics, and cosmology. This text involves the student in this rapidly growing field of research. - ;The last years have seen a symbiosis of the fields of elementary particle physics and the astrophysics of the early universe. This text presents the background of the subjects and the latest developments at a level suitable for final year undergraduates and beginning graduate students. The first chapters cover the properties and interactions of elementary"]