Name: Gravitational Waves (High Energy Physics, Cosmology and Gravitation) (en Inglés)
SKU: 55635176
Price: 1985.75 MXN
Availability: InStock
Author: Ciufolini, I.
ISBN: 9780367397609

portada Gravitational Waves (High Energy Physics, Cosmology and Gravitation) (en Inglés)

Gravitational Waves (High Energy Physics, Cosmology and Gravitation) (en Inglés)

Formato

Libro Físico

Editorial

Crc Pr Inc

Autor

Ciufolini, I.

Idioma

Inglés

Encuadernación

Tapa Blanda

ISBN13

9780367397609

Gravitational Waves (High Energy Physics, Cosmology and Gravitation) (en Inglés)

Ciufolini, I. (Autor) · Crc Pr Inc · Tapa Blanda

Libro Nuevo Importado

Envío: 22 a 27 días háb.

$ 3,309.58$ 1,985.75

-40%

Costos de importación incluídos en el precio ✅

Libro Nuevo

Quedan más de 100 unidades

$ 1,985.75

¡Envío Gratis! Llega entre el 08 Oct y el 16 Oct a CUAUHTÉMOC, Ciudad de México. Seleccionar ubicación

Agregar a lista de deseos

Reseña del libro "Gravitational Waves (High Energy Physics, Cosmology and Gravitation) (en Inglés)"

Gravitational waves (GWs) are a hot topic and promise to play a central role in astrophysics, cosmology, and theoretical physics. Technological developments have led us to the brink of their direct observation, which could become a reality in the coming years. The direct observation of GWs will open an entirely new field: GW astronomy. This is expected to bring a revolution in our knowledge of the universe by allowing the observation of previously unseen phenomena, such as the coalescence of compact objects (neutron stars and black holes), the fall of stars into supermassive black holes, stellar core collapses, big-bang relics, and the new and unexpected. With a wide range of contributions by leading scientists in the field, Gravitational Waves covers topics such as the basics of GWs, various advanced topics, GW detectors, astrophysics of GW sources, numerical applications, and several recent theoretical developments. The material is written at a level suitable for postgraduate students entering the field.