Advances in Gravitational Waves

Gravitational waves are ripples in the curvature of spacetime that propagate as waves, generated in certain gravitational interactions that propagate outward from their source. The possibility of gravitational waves was discussed in 1893 by Oliver Heaviside using the analogy between the inverse-square law in gravitation and electricity. Predicted in 1916 by Albert Einstein on the basis of his theory of general relativity, gravitational waves transport energy as gravitational radiation, a form of radiant energy similar to electromagnetic radiation.  Gravitational-wave astronomy is an emerging branch of observational astronomy which aims to use gravitational waves to collect observational data about objects such as neutron stars and black holes, events such as supernovae, and processes including those of the early universe shortly after the Big Bang.

In the present book, twelve typical literatures about gravitational waves published on international authoritative journals were selected to introduce the worldwide newest progress, which contains reviews or original researches astronomy, gravity, black holes, effect of gravitation, ect. We hope this book can demonstrate advances in gravitational waves as well as give references to the researchers, students and other related people.

Components of the Book:
  • Chapter 1
    Detection of Gravitational Waves from Black Holes: Is There a Window for Alternative Theories?
  • Chapter 2
    Friction in Gravitational Waves: Atest for Early-Time Modified Gravity
  • Chapter 3
    Gravitational Waves from First Order Phase Transitions as a Probe Ofanearly Matter Domination Era and Its Inverse Problem
  • Chapter 4
    Gravitational-Wave Mediated Preheating
  • Chapter 5
    Superconducting Antenna Concept for Gravitational Waves
  • Chapter 6
    The Speed of Gravitational Waves in Brane-worlds
  • Chapter 7
    Inflationary Gravitational Waves in Collapse Scheme Models
  • Chapter 8
    Variable Speed of Light Cosmology, Primordial Fluctuations and Gravitational Waves
  • Chapter 9
    Modeling a Nonperturbative Spinor Vacuum Interacting with a Strong Gravitational Wave
  • Chapter 10
    Thermal Noise in BEC-Phononic Gravitational Wave Detectors
  • Chapter 11
    Analog Quantum Simulation of Gravitational Waves in a Bose-Einstein Condensate
  • Chapter 12
    Testing the Kerr Black Hole Hypothesis: Comparison between the gravitational Wave and the Iron Line Approaches
Readership: Students, academics, teachers and other people attending or interested in Gravitational Waves.
Roman Konoplya
Institute for Theoretical Physics, Goethe University, Frankfurt, Germany

Valeria Pettorino
Institut für Theoretische Physik, Universit?t Heidelberg, Heidelberg, Germany

Stephon Alexander
Center for Cosmic Origins and Department of Physics and Astronomy, Dartmouth College, Hanover, New Hampshire, USA

Mauro Mariani
Facultad de Ciencias Astronómicas y Geofísicas, Universidad Nacional de La Plata, La Plata, Argentina

J. W. Moffat
Department of Physics and Astronomy, University of Waterloo, Waterloo, Ontario, Canada

Tupac Bravo
School of Mathematical Sciences, University of Nottingham, Nottingham, UK

and more...
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