Lecture Notes for PHYS 4202/5402 Cosmology - Carleton University

One of the first major events in this timeline is cosmic inflation, a rapid expansion that occurred fractions of a second after the Big Bang.







Introduction to the Theory of Relativity and Cosmology
Adopting the Planck parameters, we see this quasar barely 690 Myr after the big bang, no more than several hundred Myr after the transition from Pop III to Pop ...
Exploring the primordial universe, inflation and primordial ...
.0002 and trace amounts (of the order of 10?5) of Deuterium/H and 3He/H formed about 3 min after the Big Bang, using the latest Planck ...
George F. Smoot III - Nobel Lecture
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Could time be logarithmic? - The Journal of Cosmology
timeline
Lecture Note: Cosmology II
Termes manquants :
Early galaxy formation and its large-scale effects
Standard big bang nucleosynthesis production of H, He, Li, Be, and. B isotopes as a function of time, for the baryon density taken from WMAP7.
The hot, early universe - Haus der Astronomie
TdS = Td(sa3) = d(?a3) + Pda3. (2.8) ... properties than the classical theory: this particularity allows us to get rid of the Big Bang.
Impacts of cosmic inhomogeneities on the CMB
Big Bang. < 10-43 sec. ~infinity. All four forces (Gravity, Strong, Electromagnetic, and Weak) are united. Quantum Gravity Era. ~ 10-43 sec.
Heavy-ion Physics and the ALICE Experiment - CERN Indico
Sep 24: Introduction and Friedmann Equations. Oct 1: Fluid and Acceleration Equations. Oct 8: Introductory GR, Space Time Metric, Proper Distance.
Origins & Evolution of the Universe
Big Bang Nucleosynthesis (BBN) describes a crucial period in the early stages of our Universe. According to this theory, in a matter of ...
Probing New Physics with Big Bang Nucleosynthesis - SFB 1258
Part II: The thermal universe: This part discusses the evolution of particles in the early universe up to a time of 380,000 years after the big bang.
ASTR/PHY 395 - Cosmology - Lehigh University
Big Bang Nucleosynthesis (BBN) begins in earnest when the. Universe is a few minutes old and ends less than half an hour later when the nuclear reactions are ...