scholarly journals From crystal color symmetry to quantum spacetime

Author(s):  
Martin Bojowald ◽  
Avadh Saxena
2019 ◽  
Author(s):  
Matheus Pereira Lobo

This article addresses the connection of the UNCERTAINTY PRINCIPLE with the WIGNER FUNCTION.


2013 ◽  
Vol 28 (10) ◽  
pp. 1350035 ◽  
Author(s):  
I. V. FROLOV ◽  
M. V. MARTYNOV ◽  
A. D. SMIRNOV

The contributions of G′-boson predicted by the chiral color symmetry of quarks to the charge asymmetry [Formula: see text] in [Formula: see text]-production at the LHC and to the forward–backward asymmetry [Formula: see text] in [Formula: see text]-production at the Tevatron are calculated and analyzed in dependence on two free parameters of the model, the G′ mass mG′ and mixing angle θG. The mG′ - θG regions of 1 σ consistency with the CMS data on the cross-section [Formula: see text] and on the charge asymmetry [Formula: see text] are found and compared with those resulted from the CDF data on the cross-section [Formula: see text] and on the forward–backward asymmetry [Formula: see text] of [Formula: see text]-production at the Tevatron with account of the current SM predictions for [Formula: see text].


1996 ◽  
pp. 475-517
Author(s):  
David Ritz Finkelstein
Keyword(s):  

2003 ◽  
Vol 12 (09) ◽  
pp. 1633-1639 ◽  
Author(s):  
GIOVANNI AMELINO-CAMELIA

Over the last few years the study of possible Planck-scale departures from classical Lorentz symmetry has been one of the most active areas of quantum-gravity research. We now have a satisfactory description of the fate of Lorentz symmetry in the most popular noncommutative spacetimes and several studies have been devoted to the fate of Lorentz symmetry in loop quantum gravity. Remarkably there are planned experiments with enough sensitivity to reveal these quantum-spacetime effects, if their magnitude is only linearly suppressed by the Planck length. Unfortunately, in some quantum-gravity scenarios even the strongest quantum-spacetime effects are suppressed by at least two powers of the Planck length, and many authors have argued that it would be impossible to test these quadratically-suppressed effects. I here observe that advanced cosmic-ray observatories and neutrino observatories can provide the first elements of an experimental programme testing the possibility of departures from Lorentz symmetry that are quadratically Planck-length suppressed.


2013 ◽  
Vol 16 (1) ◽  
Author(s):  
Giovanni Amelino-Camelia
Keyword(s):  

2007 ◽  
Vol 3 (2) ◽  
pp. 81-83 ◽  
Author(s):  
Giovanni Amelino-Camelia
Keyword(s):  

2007 ◽  
Vol 22 (04) ◽  
pp. 259-271 ◽  
Author(s):  
YUE-LIANG WU

Based on a maximally symmetric minimal unification hypothesis and a quantum charge-dimension correspondence principle, it is demonstrated that each family of quarks and leptons belongs to the Majorana–Weyl spinor representation of 14 dimensions that relate to quantum spin-isospin-color charges. Families of quarks and leptons attribute to a spinor structure of extra six dimensions that relate to quantum family charges. Of particular, it is shown that ten dimensions relating to quantum spin-family charges form a motional ten-dimensional quantum spacetime with a generalized Lorentz symmetry SO (1, 9), and ten dimensions relating to quantum isospin-color charges become a motionless ten-dimensional quantum intrinsic space. Its corresponding 32-component fermions in the spinor representation possess a maximal gauge symmetry SO (32). As a consequence, a maximally symmetric minimal unification model SO (32) containing three families in ten-dimensional quantum spacetime is naturally obtained by choosing a suitable Majorana–Weyl spinor structure into which quarks and leptons are directly embedded. Both resulting symmetry and dimensions coincide with those of type I string and heterotic string SO (32) in string theory.


2018 ◽  
Vol 48 (9) ◽  
pp. 1038-1060 ◽  
Author(s):  
Yuri Bonder ◽  
Chryssomalis Chryssomalakos ◽  
Daniel Sudarsky
Keyword(s):  

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