Electron degeneracy pressure is a particular manifestation of the more general phenomenon of quantum degeneracy pressure. The Pauli exclusion principle disallows two identical half-integer spin particles (electrons and all other fermions) from simultaneously occupying the same quantum state. The result is an emergent pressure against compression of matter into smaller volumes of space. Electron degeneracy pressure results from the same underlying mechanism that defines the electron orbital structure of elemental matter. For bulk matter with no net electric charge, the attraction between electrons and nuclei exceeds (at any scale) the mutual repulsion of electrons plus the mutual repulsion of nuclei; so in absence of electron degeneracy pressure, the matter would collapse into a single nucleus. In 1967, Freeman Dyson showed that solid matter is stabilized by quantum degeneracy pressure rather than electrostatic repulsion. Because of this, electron degeneracy creates a barrier to the gravitational collapse of dying stars and is responsible for the formation of white dwarfs. (Wikipedia).
Absolute Pressure vs Gauge Pressure - Fluid Mechanics - Physics Problems
This physics video tutorial provides a basic introduction into absolute pressure and gauge pressure. The gauge pressure is the difference between the absolute pressure and the atmospheric pressure. A positive gauge pressure means the absolute pressure is above the atmospheric pressure.
From playlist New Physics Video Playlist
Chemistry - Solutions (25 of 53) Effects of Pressure on Solubility: Ex. 2
Visit http://ilectureonline.com for more math and science lectures! CORRECT VIDEO: https://www.youtube.com/watch?v=McSNIf1e-r8
From playlist CHEMISTRY 19 SOLUTIONS
Astronomy: The Supernova (5 of 10) Electron Degeneracy
Visit http://ilectureonline.com for more math and science lectures! In this video I will explain the relationship between electron degeneracy and white dwarfs.
From playlist ASTRONOMY 20 SUPERNOVA - THE DEATH OF STARS
Physics 32.5 Statistical Thermodynamics (35 of 39) What is a Degenerate Quantum State?
Visit http://ilectureonline.com for more math and science lectures! To donate: http://www.ilectureonline.com/donate https://www.patreon.com/user?u=3236071 When particles are fined to a “container” they will experience quantum states (various ways in which they can be arranged). When diff
From playlist THE "WHAT IS" PLAYLIST
Irrigation Efficiencies - Part 1
From playlist TEMP 1
Astronomy - Ch. 22: Neutron Star (3 of 17) What is Neutron Degeneracy?
Visit http://ilectureonline.com for more math and science lectures! To donate: http://www.ilectureonline.com/donate https://www.patreon.com/user?u=3236071 We will learn neutron degeneracy pressure can uphold a neutron star with a mass up to 0.7 time mass of our Sun. Two neutrons with the
From playlist THE "WHAT IS" PLAYLIST
Pedagogical Lectures on Stellar Theory - 1 by Dipankar Bhattacharya
PROGRAM VIRTUAL MEETING ON COMPACT STARS AND QCD 2020 (ORIGINALLY "COMPACT STARS IN THE QCD PHASE DIAGRAM VIII: THE ERA OF MULTI-MESSENGER ASTRONOMY") ORGANIZERS: Manjari Bagchi, Sarmistha Banik, Sudip Bhattacharyya, Prashanth Jaikumar, V. Ravindran and Sayantan Sharma DATE : 17 August
What is the Chandrasekhar limit for White Dwarf Stars?
This video provides a simplified step by step derivation of the Chandrasekhar limit for White Dwarf stars. After briefly discussing the history of white dwarf stars, an overview of electron degeneracy pressure is provided. Using a combination of quantum mechanics and Einstein's theory of s
From playlist Relativity
Physics - Thermodynamics: (7 of 22) Change Of State: Constant Pressure (Isobaric) Ex. 1
Visit http://ilectureonline.com for more math and science lectures! In this video I will give an example of an isobaric (constant) process.
From playlist PHYSICS - THERMODYNAMICS
When Quantum Physics and Relativity Compete Against Each Other to Keep Stars From Collapsing
Go to Squarespace.com for a free trial, and when you’re ready to launch, go to http://www.squarespace.com/parthg to save 10% off your first purchase of a website or domain. #degeneracypressure #quantum #neutronstar In this video, we'll be looking at degeneracy pressure - a quantum mecha
From playlist Quantum Physics by Parth G
Pedagogical Lectures on Stellar Theory - 2 by Dipankar Bhattacharya
PROGRAM VIRTUAL MEETING ON COMPACT STARS AND QCD 2020 (ORIGINALLY "COMPACT STARS IN THE QCD PHASE DIAGRAM VIII: THE ERA OF MULTI-MESSENGER ASTRONOMY") ORGANIZERS: Manjari Bagchi, Sarmistha Banik, Sudip Bhattacharyya, Prashanth Jaikumar, V. Ravindran and Sayantan Sharma DATE: 17 August
Pedagogical Lectures on Stellar Theory - 3 by Dipankar Bhattacharya
PROGRAM VIRTUAL MEETING ON COMPACT STARS AND QCD 2020 (ORIGINALLY "COMPACT STARS IN THE QCD PHASE DIAGRAM VIII: THE ERA OF MULTI-MESSENGER ASTRONOMY") ORGANIZERS: Manjari Bagchi, Sarmistha Banik, Sudip Bhattacharyya, Prashanth Jaikumar, V. Ravindran and Sayantan Sharma DATE: 17 August
8.02x - Module 02.01 - Electron Moving in an Electric Field.
Electron Moving in E-field
From playlist 8.02x - MIT Help Sessions
How Quantum Mechanics Holds Up a Dead Star - Ask a Spaceman!
Support the show: http://www.patreon.com/pmsutter All episodes: http://www.AskASpaceman.com Like on Facebook: http://www.facebook.com/PaulMattSutter How does degeneracy pressure work? What kinds of particles exist below the level of neutrons? Can they hold up a star against gravity? I di
From playlist What Fraser's watching
Chemistry - Chemical Bonding (6 of 35) Electronegativity - Definition
Visit http://ilectureonline.com for more math and science lectures! In this video I will give the definition and equation of electronegativity.
From playlist CHEMISTRY 13 LEWIS STRUCTURES
Late Stages of Evolution | Introductory Astronomy Course 8.08
Welcome to Astronomy: Exploring Time and Space, a course from Professor Impey, a University Distinguished Professor of Astronomy at the University of Arizona. Learn about the foundations of astronomy in this free online course here on YouTube. This video is part of module 8, Stars. Want t
From playlist Introductory Astronomy Module 8: Stars
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First of several videos from our Black Hole interviews. Featuring Omar Almaini, Ed Copeland, Tony Padilla, Meghan Gray and Mike Merrifield from the University of Nottingham. Playlist (more to be added soon): http://bit.ly/Black_Hole_Videos Visit our website at http://www.sixtysymbols.com/
From playlist Ed Copeland - Sixty Symbols
Electric Field (2 of 3) Calculating the Magnitude and Direction of the Electric Field
Explains how to calculate the electric field of a charged particle and the acceleration of an electron in the electric field. You can see a listing of all my videos at my website, http://www.stepbystepscience.com An electric field is an area that surrounds an electric charge, and exerts f
From playlist Electricity and Magnetism