Fitting Supernovae and Gamma Ray Bursts Data DEDGP DocumentsThis material has 4 associated documents. Select a document title to view a document's information. Main DocumentFitting Supernovae and Gamma Ray Bursts Data Model
written by
Jacob Moldenhauer, Keenan Stone, Zeke Shuler, and Larry Engelhardt The 1998 discovery of the cosmic acceleration with supernovae was recently awarded the 2011 Nobel Prize in Physics. Gamma-Ray Bursts (GRB) support this accelerated expansion of the universe (cosmic acceleration) at high redshifts up to z=8.1. The simulation allows users to compare and fit theoretical models of cosmology with recent gamma-ray bursts data sets to confirm the accelerated expansion of the universe. This modeling allows the user to vary cosmological parameters within a particular class of dark energy cosmological models to fit a particular cosmological data set. The user can plot several theoretical curves with the data to compare different models. The values of these parameters, for a particular model, determine the physical description and evolution of the universe.
Published August 11, 2012
This file has previous versions. Supplemental DocumentsGamma Ray Burst Data ModelThe Gamma Ray Burst Data Model allows the user to test a cosmological model with different data sets.
Last Modified November 18, 2012
This file has previous versions. Source Code Documents (2)Fitting Supernovae and Gamma Ray Bursts Data Source CodeThe source code zip archive contains an XML representation of the Fitting Supernovae and Gamma Ray Bursts Data Model. Unzip this archive in your EJS workspace to compile and run this model using EJS.
Last Modified August 17, 2017
This file has previous versions. Gamma Ray Burst Data Source CodeThe source code zip archive contains an EJS-XML representation of the Gamma Ray Burst Data Model. Unzip this archive in your EJS workspace to compile and run this model using EJS.
Last Modified November 18, 2012
This file has previous versions. |