Advances in Astrophysics
Size of the Observable Universe
Download PDF (393.8 KB) PP. 135 - 137 Pub. Date: November 1, 2016
Author(s)
- Paul Halpern*
Dept. of Math, Physics, and Statistics, University of the Sciences in Philadelphia, 600 S. 43rd St., Philadelphia, PA, United States - Nick Tomasello*
Dept. of Math, Physics, and Statistics, University of the Sciences in Philadelphia, 600 S. 43rd St., Philadelphia, PA, United States
Abstract
Keywords
References
[1] A. G. Riess, et. al., “Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant,” Astronomical Journal, vol. 116, pp. 1009–1038, 1998.
[2] S. Perlmutter, et. al., “Measurements of Omega and Lambda from 42 High-Redshift Supernovae,” Astrophysical Journal, vol. 517, pp. 565–586, 1999.
[3] T. M. Davis and C. H. Lineweaver, “Expanding Confusion: Common Misconceptions of Cosmological Horizons and the Superluminal Expansion of the Universe,” Publications of the Astronomical Society of Australia, vol. 21, pp. 97–109, 2004.
[4] J. R. Gott III, et. al., “A Map of the Universe,” Astronomical Journal, vol. 624, pp. 463–484, 2005.
[5] D. N. Spergel, et. al., “First year Wilkinson Microwave Anisotropy Probe (WMAP) observations: determination of cosmological parameters,” Astronomical Journal Supplement, vol. 148, pp. 175–194, 2003.
[6] P. A. R. Ade, et. al., “Planck 2013 results. XVI. Cosmological Parameters ,” Astronomy and Astrophysics, vol. 571, no. A16, pp. 1–66, 2014. 7. P. A. R. Ade, et. al., “Planck 2015 results. XIII. Cosmological parameters,” ArXiv:1502.01589. Accepted for publication in Astronomical Journal, 2016.