Journal of Undergraduate Research
Keywords
modeling magnetized, rotating neutron stars, axisymmetry
College
Physical and Mathematical Sciences
Department
Physics and Astronomy
Abstract
There has been a tremendous research effort in trying to understand observed astrophysical phenomena. The difficulties in studying the formation of and interactions between astrophysical objects have led to the use of computational methods to solve these problems. From a theoretical point of view, one difficulty is that many of these problems have no known exact solution and therefore approximations have to be made. Computers can handle these approximations well and since they can perform many operations quickly, we can find greater accuracy by utilizing them. Once a good mathematical model is generated for some astrophysical object (say black holes, galaxies or stars) researchers can investigate stability, formation or collision of these objects with other interstellar objects. These models can be used to understand how a solar system, galaxy or even the whole universe was formed and how it will continue to change.
Recommended Citation
Greenwald, Jared and Hirschmann, Dr. Eric
(2013)
"Modeling Magnetized, Differentially Rotating Neutron Stars,"
Journal of Undergraduate Research: Vol. 2013:
Iss.
1, Article 2766.
Available at:
https://scholarsarchive.byu.edu/jur/vol2013/iss1/2766