Chromogravity explains {open_quotes}strong gravity{close_quotes}

Technical Report · Mon Mar 01 04:00:00 EST 1993

DOI:https://doi.org/10.2172/10138036· OSTI ID:10138036

Ne`eman, Y ^[1]; Sijacki, D ^[2]

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1. Tel-Aviv Univ. (Israel). Sackler Faculty of Exact Sciences
2. Institute of Physics, Belgrade (Yugoslavia)

In this paper the authors deal with the question of gravitational type interactions in the case of strong interaction phenomena. They present arguments which indicate that it is not necessary to invoke a gravity type interaction into QCD in order to account for observed phenomena. They argue that the gravitational type phenomena discussed in previous work is a manifestation of a class of Feynmann diagrams. These seem to generate an analog to gravity, a J=2 {open_quotes}chromograviton{close_quotes} or {open_quotes}pseudo-graviton{close_quotes} whose action effectively generates Salam`s {open_quotes}Strong Gravity{close_quotes} or {open_quotes}f-gravity{close_quotes}, withthough having to introduce the theory as an additional input.

• Research Organization: Texas Univ., Austin, TX (United States). Center for Particle Physics
• Sponsoring Organization: USDOE, Washington, DC (United States)
• DOE Contract Number: FG05-85ER40200
• OSTI ID: 10138036
• Report Number(s): DOE/ER/40200--324; TAUP/N--228-93; ON: DE94009184
• Country of Publication: United States
• Language: English

Related Subjects

662230
662240
72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
INTERACTION RANGE
MODELS FOR STRONG INTERACTIONS
QUANTUM CHROMODYNAMICS
QUANTUM GRAVITY
STRONG INTERACTIONS