EconPapers    
Economics at your fingertips  
 

The emergence of free energy

George Marx

Physica A: Statistical Mechanics and its Applications, 1995, vol. 221, issue 1, 361-371

Abstract: The early Universe was hot and dense, with frequent collisions. Therefore it was in thermal equilibrium, as indicated by the properties of the observed relic black body radiation. Consequently the free energy of the early Universe was zero. Our present world, however, is out of equilibrium; it is locally alive. One has to find places and epochs in the Universe where free energy is being created or stored.

Date: 1995
References: View complete reference list from CitEc
Citations:

Downloads: (external link)
http://www.sciencedirect.com/science/article/pii/037843719500227X
Full text for ScienceDirect subscribers only. Journal offers the option of making the article available online on Science direct for a fee of $3,000

Related works:
This item may be available elsewhere in EconPapers: Search for items with the same title.

Export reference: BibTeX RIS (EndNote, ProCite, RefMan) HTML/Text

Persistent link: https://EconPapers.repec.org/RePEc:eee:phsmap:v:221:y:1995:i:1:p:361-371

DOI: 10.1016/0378-4371(95)00227-X

Access Statistics for this article

Physica A: Statistical Mechanics and its Applications is currently edited by K. A. Dawson, J. O. Indekeu, H.E. Stanley and C. Tsallis

More articles in Physica A: Statistical Mechanics and its Applications from Elsevier
Bibliographic data for series maintained by Catherine Liu ().

 
Page updated 2025-03-19
Handle: RePEc:eee:phsmap:v:221:y:1995:i:1:p:361-371