Gravitational-Wave Astronomy: Exploring the Dark Side of the Universe: Oxford Graduate Texts
Autor Nils Anderssonen Limba Engleză Paperback – 20 noi 2025
| Toate formatele și edițiile | Preț | Express |
|---|---|---|
| Paperback (1) | 348.33 lei 20-31 zile | |
| OUP OXFORD – 20 noi 2025 | 348.33 lei 20-31 zile | |
| Hardback (1) | 560.38 lei 41-52 zile | |
| OUP OXFORD – 28 noi 2019 | 560.38 lei 41-52 zile |
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Specificații
ISBN-13: 9780198989097
ISBN-10: 0198989091
Pagini: 688
Ilustrații: 116 color and 51 grayscale line figures; 1 color halftone
Dimensiuni: 175 x 246 x 34 mm
Greutate: 1.32 kg
Editura: OUP OXFORD
Colecția OUP Oxford
Seria Oxford Graduate Texts
Locul publicării:Oxford, United Kingdom
ISBN-10: 0198989091
Pagini: 688
Ilustrații: 116 color and 51 grayscale line figures; 1 color halftone
Dimensiuni: 175 x 246 x 34 mm
Greutate: 1.32 kg
Editura: OUP OXFORD
Colecția OUP Oxford
Seria Oxford Graduate Texts
Locul publicării:Oxford, United Kingdom
Recenzii
This book is a wonderful introduction to one of the most exciting research areas in modern physics (gravitational wave astronomy) written by a leading expert on the structure and dynamics of black holes and neutron stars....The book is an excellent resource for students and for researchers working in specific areas (general relativity, astronomy, data analysis, nuclear and particle physics) who may want to put their work in a broader context.
Notă biografică
Nils Andersson is a professor of mathematics and an expert on Einstein's theory of relativity and related astrophysics. He is an elected honorary Fellow of the International Society on General Relativity and Gravitation and was awarded the 2024 Karl Schwarzschild Prize in astrophysics. His research mainly concerns black holes, neutron stars and gravitational waves. Over the last couple of decades, he has actively pursued many issues relevant to the emerging area of gravitational-wave astronomy. His current work focuses on the extreme physics that neutron stars represent, from the state and composition of matter to the dynamical role of the superfluid and superconducting components expected to be present in the core of a mature neutron star.