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The top documents tagged [degenerate electron]

The Quantized Free Electron Theory ++++++++ Energy E Spatial coordinate x Nucleus with localized core electrons Jellium model: electrons shield potential
The Quantized Free Electron Theory ++++++++ Energy E Spatial coordinate x Nucleus with localized core electrons Jellium model: electrons shield potential
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White Dwarfs and Novae – The Vampire Stars. What’s a White Dwarf Like? Same size as the earth to slightly larger. Very hot – surface temperatures of up
White Dwarfs and Novae – The Vampire Stars. What’s a White Dwarf Like? Same size as the earth to slightly larger. Very hot – surface temperatures of up
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quTpdf (quantum transport notes)
quTpdf (quantum transport notes)
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Galperin Y.M.-introduction to Modern Solid State Physics (2001)
Galperin Y.M.-introduction to Modern Solid State Physics (2001)
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White Dwarfs, Novae, and Type 1a Supernovae: The Vampire Stars Ohio University - Lancaster Campus slide 1 of 64 Spring 2009 PSC 100
White Dwarfs, Novae, and Type 1a Supernovae: The Vampire Stars Ohio University - Lancaster Campus slide 1 of 64 Spring 2009 PSC 100
219 views
Pulsars + Parkes = Awesome Ryan Shannon Postdoctoral Fellow, CSIRO Astronomy and Space Science Credit: John Sarkissian
Pulsars + Parkes = Awesome Ryan Shannon Postdoctoral Fellow, CSIRO Astronomy and Space Science Credit: John Sarkissian
216 views
Electrons in metals ++++++++ Energy E Spatial coordinate x Nucleus with localized core electrons Jellium model: electrons shield potential to a large extent
Electrons in metals ++++++++ Energy E Spatial coordinate x Nucleus with localized core electrons Jellium model: electrons shield potential to a large extent
227 views
1 As hydrogen is exhausted in the (convective) core of a star (point 2) it moves away from the main sequence (point 3) What happens to the star ? lower
1 As hydrogen is exhausted in the (convective) core of a star (point 2) it moves away from the main sequence (point 3) What happens to the star ? lower
216 views
Chapter 20 part 1: Star death: –0.4 - 4 M Carbon White dwarfs –> 4 M Supernova SN1987A Neutrinos –Supernovae involving white dwarfs –Supernova remnants
Chapter 20 part 1: Star death: –0.4 - 4 M Carbon White dwarfs –> 4 M Supernova SN1987A Neutrinos –Supernovae involving white dwarfs –Supernova remnants
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Super Massive Black Holes A Talk Given By: Mike Ewers
Super Massive Black Holes A Talk Given By: Mike Ewers
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Dark Matter in the Center of the Milky Way and the Stars Burning It Igor V. Moskalenko & Lawrence L. Wai (Stanford, KIPAC, SLAC) M&W 2007, ApJL accepted
Dark Matter in the Center of the Milky Way and the Stars Burning It Igor V. Moskalenko & Lawrence L. Wai (Stanford, KIPAC, SLAC) M&W 2007, ApJL accepted
217 views
Lecture 23. Degenerate Fermi Gas & Bose-Einstein condensation (Ch. 7) Today’s plan: high density limit n ~ n Q 1.Fermion: Degenerate Fermi Gas (7.3) 2.Boson:
Lecture 23. Degenerate Fermi Gas & Bose-Einstein condensation (Ch. 7) Today’s plan: high density limit n ~ n Q 1.Fermion: Degenerate Fermi Gas (7.3) 2.Boson:
221 views