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Plasmas fríos moleculares en el Universo y en el laboratorio

Authors: Tanarro, Isabel;

Plasmas fríos moleculares en el Universo y en el laboratorio

Abstract

Según la energía de sus partículas, los plasmas constituyen el cuarto estado de agregación de la materia, tras sólidos, líquidos y gases. Para cambiar de uno a otro, es preciso aportar energía y aumentar la temperatura. Incrementando la temperatura en un gas considerablemente, sus átomos o moléculas adquieren energía suficiente para ionizarse al chocar entre sí, de modo que a ~ 20.000 K muchos gases presentan una ionización elevada. Sin embargo, átomos y moléculas pueden ionizarse también por impacto electrónico, absorción de fotones, reacciones químicas o nucleares, u otros procesos.

Estudios citados en el presente trabajo han recibido apoyo de los Proyectos ENE 2006-14577-C04-03, FIS 2007-61686 y CSD2009-00038 del MCI de España.

4 páginas, 2 figuras.

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
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