Add to ORKGOur ultimate goal is to model the dynamics of a compact object orbiting a large black hole. However, there is no known exact solution to the Einstein field equation and it requires application of numerous mathematical techniques. Therefore, in this project, we seek to solve the simple differential equation called wave equation in spherical coordinate. This model is analogous to Einstein’s field equation for a black hole binary system and by obtaining a three dimensional wave equation, we take a step toward a theoretical model of gravitational waves from astronomical source
The direct observation and characterization of gravitational waves from binary black-hole mergers by...
The expectation that light waves are the only way to gather information about the distant universe d...
We present a finite difference version of the eth formalism, which allows use of tensor fields in sp...
Our ultimate goal is to model the dynamics of a compact object orbiting a large black hole. However,...
Our ultimate goal is to compute the gravitational waves in an extreme mass-ratio binary system. Sinc...
Gravitational waves are produced by orbiting massive binary objects, such as black holes and neutron...
We present the metric appropriate to a spherical shock wave in the framework of general relativity. ...
[eng] The first detection of a gravitational wave signal occurred on September 14 2015, when the tw...
[eng] This thesis concerns the gravitational wave signal emitted by merging black holes, as is descr...
We consider a compact source of gravitational waves of frequency, in or near a massive spherically s...
Using only Newtonian gravity and a little special relativity we calculate most of the important effe...
The gravitational waves produced by the inspiral and merger of two black holes are expected to be th...
There is continuing interest in the numerical solution of the field equations of general relativity....
This thesis concerns the use of observations of gravitational waves as tools for astronomy and funda...
Recent interesting astrophysical observations point towards a multi-messenger, multi-wavelength appr...
The direct observation and characterization of gravitational waves from binary black-hole mergers by...
The expectation that light waves are the only way to gather information about the distant universe d...
We present a finite difference version of the eth formalism, which allows use of tensor fields in sp...
Our ultimate goal is to model the dynamics of a compact object orbiting a large black hole. However,...
Our ultimate goal is to compute the gravitational waves in an extreme mass-ratio binary system. Sinc...
Gravitational waves are produced by orbiting massive binary objects, such as black holes and neutron...
We present the metric appropriate to a spherical shock wave in the framework of general relativity. ...
[eng] The first detection of a gravitational wave signal occurred on September 14 2015, when the tw...
[eng] This thesis concerns the gravitational wave signal emitted by merging black holes, as is descr...
We consider a compact source of gravitational waves of frequency, in or near a massive spherically s...
Using only Newtonian gravity and a little special relativity we calculate most of the important effe...
The gravitational waves produced by the inspiral and merger of two black holes are expected to be th...
There is continuing interest in the numerical solution of the field equations of general relativity....
This thesis concerns the use of observations of gravitational waves as tools for astronomy and funda...
Recent interesting astrophysical observations point towards a multi-messenger, multi-wavelength appr...
The direct observation and characterization of gravitational waves from binary black-hole mergers by...
The expectation that light waves are the only way to gather information about the distant universe d...
We present a finite difference version of the eth formalism, which allows use of tensor fields in sp...