Computation of the polarization creep tensor
The fourth-rank tensor, which appears in the linear relationship between the creep velocity produced by a polarization flux and the flux itself, is computed as a function of the magnetic field and the molecular constants of the polyatomic gas where the phenomenon occurs. Numerical values are given for the typical case of N2.
Year of publication: |
1983
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Authors: | Cercignani, C. ; Geppert, L. ; Lampis, M. |
Published in: |
Physica A: Statistical Mechanics and its Applications. - Elsevier, ISSN 0378-4371. - Vol. 121.1983, 3, p. 531-540
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Publisher: |
Elsevier |
Saved in:
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