RELATIVITY GROUPOID INSTEAD OF RELATIVITY GROUP

Author:

OZIEWICZ ZBIGNIEW1

Affiliation:

1. Universidad Nacional Autónoma de México, Facultad de Estudios Superiores Cuautitlán, Apartado Postal # 25, C.P. 54714 Cuautitlán Izcalli, Estado de México, México

Abstract

In 1908, Minkowski [13] used space-like binary velocity-field of a medium, relative to an observer. In 1974, Hestenes introduced, within a Clifford algebra, an axiomatic binary relative velocity as a Minkowski bivector [7, 8]. We propose to consider binary relative velocity as a traceless nilpotent endomorphism in an operator algebra. Any concept of a binary axiomatic relative velocity made possible the replacement of the Lorentz relativity group by the relativity groupoid. The relativity groupoid is a category of massive bodies in mutual relative motions, where a binary relative velocity is interpreted as a categorical morphism with the associative addition. This associative addition is to be contrasted with non-associative addition of (ternary) relative velocities in isometric special relativity (loop structure). We consider an algebra of many time-plus-space splits, as an operator algebra generated by idempotents. The kinematics of relativity groupoid is ruled by associative Frobenius operator algebra, whereas the dynamics of categorical relativity needs the non-associative Frölicher–Richardson operator algebra. The Lorentz covariance is the cornerstone of physical theory. Observer-dependence within relativity groupoid, and the Lorentz-covariance within the Lorentz relativity group, are different concepts. Laws of Physics could be observer-free, rather than Lorentz-invariant.

Publisher

World Scientific Pub Co Pte Lt

Subject

Physics and Astronomy (miscellaneous)

Reference16 articles.

1. Relative observer kinematics in general relativity

2. J. J. Cruz and Z. Oziewicz, Non-Associative Algebra and Its Applications, eds. L. Sabinin, L. Sbitneva and I. Shestakov (Chapman & Hall/CRC Press, Boca Raton, London, 2006) pp. 109–127.

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