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Lecture 3 Composition of the Universe | Relativistic Cosmology Part 2
Lecture 3 Composition of the Universe | Relativistic Cosmology Part 2

4- Cosmology - II
4- Cosmology - II

Dark Energy and the Accelerating Universe - J.A. Frieman et al.
Dark Energy and the Accelerating Universe - J.A. Frieman et al.

Universe | Free Full-Text | Unified Description of Dark Energy and Dark  Matter within the Generalized Hybrid Metric-Palatini Theory of Gravity
Universe | Free Full-Text | Unified Description of Dark Energy and Dark Matter within the Generalized Hybrid Metric-Palatini Theory of Gravity

The Early Universe
The Early Universe

Universe | Free Full-Text | Newtonian Cosmology and Evolution of  κ-Deformed Universe
Universe | Free Full-Text | Newtonian Cosmology and Evolution of κ-Deformed Universe

The Hubble constant troubled by dark matter in non-standard cosmologies |  Scientific Reports
The Hubble constant troubled by dark matter in non-standard cosmologies | Scientific Reports

17.3: The Friedmann Equation and the Fate of the Universe - Physics  LibreTexts
17.3: The Friedmann Equation and the Fate of the Universe - Physics LibreTexts

A New Idea for How Dark Matter Came to Dominate the Universe | Inside  Science
A New Idea for How Dark Matter Came to Dominate the Universe | Inside Science

The scale factor for matter and radiation dominated universes, w = 0... |  Download Scientific Diagram
The scale factor for matter and radiation dominated universes, w = 0... | Download Scientific Diagram

1: A brief history of the Universe with a focus on the domination of... |  Download Scientific Diagram
1: A brief history of the Universe with a focus on the domination of... | Download Scientific Diagram

matter era and beyond
matter era and beyond

Cosmology - Matter Dominated Universe
Cosmology - Matter Dominated Universe

Expanding Universe
Expanding Universe

SOLVED: In a flat and matter-dominated universe, assume that dark energy  changes with zD/√V = V a. Show that the continuity equation (fluid  equation) takes its form ∇⋅(Ï m0v) + 3Pm0H =
SOLVED: In a flat and matter-dominated universe, assume that dark energy changes with zD/√V = V a. Show that the continuity equation (fluid equation) takes its form ∇⋅(Ï m0v) + 3Pm0H =

Chapter 27, Section 1
Chapter 27, Section 1

Matter-Dominated Universe - YouTube
Matter-Dominated Universe - YouTube

Cosmological constant - Wikipedia
Cosmological constant - Wikipedia

cosmology - How did the universe shift from "dark matter dominated" to  "dark energy dominated"? - Physics Stack Exchange
cosmology - How did the universe shift from "dark matter dominated" to "dark energy dominated"? - Physics Stack Exchange

Dark Matter Less Influential in Galaxies in Early Universe | ESO
Dark Matter Less Influential in Galaxies in Early Universe | ESO

Cosmology - Radiation Dominated Universe
Cosmology - Radiation Dominated Universe

Ask Ethan: When Were Dark Matter And Dark Energy Created?
Ask Ethan: When Were Dark Matter And Dark Energy Created?

cosmology - Why does the current age of the universe increase when dark  energy is included? (open universe) - Physics Stack Exchange
cosmology - Why does the current age of the universe increase when dark energy is included? (open universe) - Physics Stack Exchange

Particle Physics in the Early Universe
Particle Physics in the Early Universe

Ask Ethan: Why doesn't radiation dominate the Universe? - Big Think
Ask Ethan: Why doesn't radiation dominate the Universe? - Big Think