Maximum acceleration and magnetic field in the early universe

dc.contributor.author	Sivaram, C
dc.contributor.author	de Sabbata, Venzo
dc.date.accessioned	2008-07-16T05:31:00Z
dc.date.available	2008-07-16T05:31:00Z
dc.date.issued	1991-02
dc.identifier.citation	Astrophysics and Space Science , Vol. 176, No. 1, pp. 145 - 148	en
dc.identifier.issn	0004-640X
dc.identifier.uri	http://hdl.handle.net/2248/2693
dc.description.abstract	The maximum acceleration at the Planck epoch is shown to be related to the maximum magnetic field and curvature as well as temperature in that era. Spin-torsion effects at that epoch also lead to same value.	en
dc.format.extent	277105 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Kluwer Academic Publishers	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1991Ap%26SS.176..145S	en
dc.relation.uri	http://www.springerlink.com/content/n87m71k7r0151106/?p=ebf6c406af654d2a884986fde28dd489&pi=13	en
dc.subject	Acceleration (Physics)	en
dc.subject	Big bang cosmology	en
dc.subject	Magnetic flux	en
dc.subject	Particle acceleration	en
dc.subject	Particle acceleration	en
dc.subject	Space-time functions	en
dc.subject	Astronomical models	en
dc.subject	Gravitational effects	en
dc.subject	Magnetic fields	en
dc.subject	Relativistic effects	en
dc.subject	Torsion	en
dc.title	Maximum acceleration and magnetic field in the early universe	en
dc.type	Article	en