Generalization of the Dissipative Model of the Universe: Difference between revisions
Appearance
Imported from text file |
infobox: unlink bare volume/issue numbers (removes redlinks to numeric titles) |
||
| Line 5: | Line 5: | ||
| published = 1993 | | published = 1993 | ||
| journal = [[Galilean Electrodynamics]] | | journal = [[Galilean Electrodynamics]] | ||
| volume = | | volume = 4 | ||
| number = | | number = 3 | ||
| pages = 51-53 | | pages = 51-53 | ||
}} | }} | ||
Latest revision as of 09:27, 21 July 2026
| Scientific Paper | |
|---|---|
| Title | Generalization of the Dissipative Model of the Universe |
| Author(s) | Pal R Molnar |
| Keywords | generalization of the dissipative model of the universe (DMU), megascopic mass flow |
| Published | 1993 |
| Journal | Galilean Electrodynamics |
| Volume | 4 |
| Number | 3 |
| Pages | 51-53 |
Abstract
The present study gives a method for the phenomenological description of megascopic mass flow of the Universe in the framework of the generalization of the Dissipative Model of the Universe (DMU) [1]. The axiomatical basis and mathematical framework of DMU will be applied and referred to.