Tag Archive for: cosmology

Spatial Curvature in Cosmological Models
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Standard cosmological models are classified by spatial curvature into three broad types: open, flat, and closed universes. These correspond to negative,…

Dark Energy Part 3: Fitting the SCP Union 2.1 Supernova Data
In Part 1 of this 3-part series, I explained kinematics in Einstien-deSitter (EdS) cosmology and in Part 2, I explained kinematics in ##\Lambda##CDM cosmology…

Dark Energy Part 2: LCDM Cosmology
This is Part 2 of a 3-part series explaining evidence for so-called “dark energy” leading to a current positive cosmological acceleration. The evidence…

Dark Energy Part 1: Einstein-deSitter Cosmology
In this 3-part series, I want to motivate the (re)introduction of the cosmological constant ##\Lambda## into Einstein's equations of general relativity…

Evidence for the Big Bang: CMB, Hubble’s Law, FAQ Guide
Big Bang: Key PointsHubble's law (redshift of galaxies) and the Doppler effect provide direct evidence that the universe is expanding away from our…

Cosmic Web Connectivity: Galaxy Evolution and Quenching
The universe was not perfectly uniform at the beginning; some regions had higher density than others. Over time these higher-density regions attracted…

Gaia Astrometry: Detecting Gravitational Waves Effectively
Gravitational waves (GWs) are disturbances in spacetime produced by massive objects moving asymmetrically. Only the most massive and most relativistic…

Why Uranus Spins on Its Side: Spin–Orbit Resonance
Uranus spins on its side. It has an obliquity (tilt) of 98° — its rotation axis lies closer to the ecliptic plane than any other planet — and astronomers…

VHE Gamma Rays from Sgr A*: Black Holes and CTA Observations
Black Hole Key PointsBlack holes (BHs) have a gravitational pull so strong that nothing, not even light, can escape.
BHs can be divided into two…

Mass Inflation Inside Black Holes — Explanation & Equations
Definition and summary
Abstract from Poisson and Israel (1990), "Internal structure of black holes":
"The gravitational effects associated with the radiative…

Equations of State for Photon Gas and Relativistic Electron Gas
This Insight develops equations of state that are useful in calculations about cosmology and about the insides of stars. The first calculation is for a…

A Formal Definition of Large-Scale Isotropy
This Insight is part of my attempt to develop a formal definition of 'large-scale isotropy', a concept that is fundamental to most cosmology, but that…

Did the Big Bang Have a Center? Explaining Cosmology
Did the Big Bang Have a Center?
What the standard models say
According to standard cosmological models based on general relativity — and which agree…

What Is the Steady-state Model and Why It’s No Longer Viable
Introduction to the Steady State Model
Back in 2011, I wrote a FAQ entry for Physics Forums on the steady state model and why it is no longer viable.…

Inflationary Misconceptions and the Basics of Cosmological Horizons
Introduction
It is a common saying that during inflation "space expanded faster than the speed of light." This statement is meant to articulate the…

Learn About Neutrino Masses and Speed
It was hard to miss the 2011 OPERA neutrino speed measurement that indicated superluminal neutrino speeds (and turned out to be a measurement error), but…
