Tectonic signatures in coseismic gravitational energy change
نویسندگان
چکیده
منابع مشابه
Gravitational Radiation Sources and Signatures
The goal of these lecture notes is to introduce the developing research area of gravitational-wave phenomenology. In more concrete terms, they are meant to provide an overview of gravitational-wave sources and an introduction to the interpretation of real gravitational wave detector data. They are, of course, limited in both regards. Either topic could be the subject of one or more books, and c...
متن کاملSignatures of extra dimensions in gravitational waves
Considering gravitational waves propagating on the most general 4+N -dimensional space-time, we investigate the effects due to the N extra dimensions on the fourdimensional waves. All wave equations are derived in general and discussed. On Minkowski4 times an arbitrary Ricci-flat compact manifold, we find: a massless wave with an additional polarization, the breathing mode, and extra waves with...
متن کاملGravitational Energy
Observers at rest in a stationary spacetime flat at infinity can measure small amounts of rest-mass+internal energies+kinetic energies+pressure energy in a small volume of fluid attached to a local inertial frame. The sum of these small amounts is the total “matter energy” EM for those observers. If Mc 2 is the total mass-energy, the difference Mc − EM is the binding gravitational energy. Misne...
متن کاملGravitational energy in stationary spacetimes
Static observers remain on Killing-vector world lines and measure the rest-mass+kinetic energies of particles moving past them, and the flux of that mechanical energy through space and time. The total mechanical energy is the total flux through a spacelike cut at one time. The difference between the total mass-energy and the total mechanical energy is the total gravitational energy, which we pr...
متن کاملGravitational energy in spherical symmetry.
Various properties of the Misner-Sharp spherically symmetric gravitational energy E are derived, and known properties reviewed. In the Newtonian limit, E yields the Newtonian mass to leading order and the Newtonian kinetic and potential energy to the next order. In vacuo, E reduces to the Schwarzschild parameter. At null and spatial infinity, E reduces to the Bondi-Sachs and Arnowitt-Deser-Misn...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
ژورنال
عنوان ژورنال: Geophysical Journal International
سال: 2002
ISSN: 0956-540X,1365-246X
DOI: 10.1046/j.1365-246x.2002.01662.x