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Hadron epoch

Scalar Correlation Functions in De Sitter Space from the Stochastic Spectral Expansion
What Did the Early Universe Look Like? Key Stage 5
Primordial Black Holes from the QCD Epoch: Linking Dark Matter
Early Universe Thermodynamics and Evolution in Nonviscous and Viscous Strong and Electroweak Epochs: Possible Analytical Solutions
Lecture 17 : the Early Universe I
16Th the Very Early Universe
Arxiv:1904.11482V1 [Astro-Ph.CO] 25 Apr 2019 Chromodynamics (QCD) Scale, Λ ≈ 200 Mev
Constraining the Hubble Parameter Using Distance Modulus – Redshift Relation
Fundamental Physics and Relativistic Laboratory Astrophysics with Extreme Power Lasers
Quarks and Hadrons – and the Spectrum in Between
Impacts of Cosmic Inhomogeneities on the CMB: Primordial Perturbations in Two-Field Bouncing Cosmologies and Cosmic Magnetism In
Cosmology: Historical Outline
Lecture 17 : the Early Universe I
Thermal History of the Universe and Early Growth of Density Fluctuations
Constraining the Hubble Parameter Using Distance Modulus-Redshift
Class 18 the Early Universe and Nucleosynthesis
The Universe; the Whole Shebang
University of Groningen Gauging the Inner Mass Power Spectrum of Early

Top View

The QCD Phase Diagram
ASTROPHYSICS I: Lecture Notes, ETH Zurich 2018
Arxiv:1611.07802V2
Decay of Baryon Inhomogeneities in an Expanding Universe
Brief Review of Cosmology Universe Is Expanding
Modelling and Machine Learning for the Epoch of Reionization
Where Astronomy Meets Particle Physics
Panel 0: Big-Bang and Cosmos, on a Logarithmic Time Scale (13.8 Ga to Now) © Walter Álvarez, 2019

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