Detecting the Stochastic Gravitational-Wave Background (häftad)
Fler böcker inom
Format
Häftad (Paperback / softback)
Språk
Engelska
Antal sidor
57
Utgivningsdatum
2017-12-30
Förlag
Morgan & Claypool Publishers
Illustrationer
Color illustrations
Dimensioner
254 x 178 x 3 mm
Vikt
118 g
Antal komponenter
1
Komponenter
1366:Standard Color 7 x 10 in or 254 x 178 mm Perfect Bound on White w/Gloss Lam
ISBN
9781681740188
Detecting the Stochastic Gravitational-Wave Background (häftad)

Detecting the Stochastic Gravitational-Wave Background

Häftad Engelska, 2017-12-30
429
Skickas inom 7-10 vardagar.
Gratis frakt inom Sverige över 159 kr för privatpersoner.
The stochastic gravitational-wave background (SGWB) is by far the most difficult source of gravitational radiation detect. At the same time, it is the most interesting and intriguing one. This book describes the initial detection of the SGWB and describes the underlying mathematics behind one of the most amazing discoveries of the 21st century. On the experimental side it would mean that interferometric gravitational wave detectors work even better than expected. On the observational side, such a detection could give us information about the very early Universe, information that could not be obtained otherwise. Even negative results and improved upper bounds could put constraints on many cosmological and particle physics models.
Visa hela texten

Passar bra ihop

  1. Detecting the Stochastic Gravitational-Wave Background
  2. +
  3. Mechanochemistry

De som köpt den här boken har ofta också köpt Mechanochemistry av Evelina Colacino, Guido Ennas, Ivan Halasz, Andrea Porcheddu, Alessandra Scano (häftad).

Köp båda 2 för 1338 kr

Kundrecensioner

Har du läst boken? Sätt ditt betyg »

Övrig information

Carlo Nicola Colacino currently holds a research position at INFN (Italian National Institute for Nuclear physics). He received his PhD from the University of Cagliari in 2001 under the supervision of Massimo Bianchi. He has conducted research at the Max-Planck-Institut for Gravitational Physics, the University of Birmingham, and the Research Institute for Nuclear and Particle Physics in Hungary. His main interest lies in gravitational-wave physics, both by studying possible sources and by participating in the LIGO Scientific Collaboration's data analysis efforts.

Innehållsförteckning

Preface Acknowledgements Author biography 1. A brief history of gravitational radiation 2. General theoretical considerations about the cosmological SGWB 3. SGWB generation and source detection 4. Astrophysical sources