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Topic: Gigakelvin


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In the News (Sun 3 Jun 12)

  
  EVWORLD FEATURE: David Sereda: Beyond Convention:SEREDA | FUSION | HE3 | HELIUM | NUCLEAR | UFO | SOLAR | SCOTT |
To do this,however, requires that the the Coulomb barrier of.1 Mev (million electron-volts) must be overcome.
To impart sufficient energy to the deuterium-tritium nuclei to accomplish this requires a temperature of 1 GK (gigakelvin).
The nuclei at this temperature become a hot gas or plasma.
www.evworld.com /view.cfm?section=article&archive=1&storyid=936&first=4188&end=4187   (4005 words)

  
  Sonoluminescence - Wikipedia, the free encyclopedia
This has led to differing estimates on the temperatures in the bubble, since they are extrapolated from the emission spectra taken during collapse, or estimated using a modified Rayleigh-Plesset equation (see below).
Some estimates put the inside of the bubble at one gigakelvin [1].
These estimates are based on models which cannot be verified at present, and may include too many unsupported assumptions.
en.wikipedia.org /wiki/Sonoluminescence   (1592 words)

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