Richard Galvez
Syracuse University
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Featured researches published by Richard Galvez.
Journal of High Energy Physics | 2012
Simon Catterall; Richard Galvez; Anosh Joseph; Dhagash Mehta
A bstractIn recent years a new class of supersymmetric lattice theories have been proposed which retain one or more exact supersymmetries for non-zero lattice spacing. Recently there has been some controversy in the literature concerning whether these theories suffer from a sign problem. In this paper we address this issue by conducting simulations of the
Physical Review D | 2014
Richard Easther; Richard Galvez; Ogan Özsoy; Scott Watson
\mathcal{N}
Journal of High Energy Physics | 2012
Simon Catterall; Poul H. Damgaard; Thomas DeGrand; Richard Galvez; Dhagash Mehta
= (2, 2) and
Journal of High Energy Physics | 2010
Simon Catterall; Richard Galvez; Mithat Unsal
\mathcal{N}
Physical Review D | 2012
Simon Catterall; Richard Galvez; Jay Hubisz; Dhagash Mehta; Aarti Veernala
= (8, 8) supersymmetric Yang-Mills theories in two dimensions for the U(N ) theories with N = 2, 3, 4, using the new twisted lattice formulations. Our results provide evidence that these theories do not suffer from a sign problem in the continuum limit. These results thus boost confidence that the new lattice formulations can be used successfully to explore non-perturbative aspects of four-dimensional
Physical Review D | 2017
Richard Galvez; Robert J. Scherrer
\mathcal{N}
Proceedings of The XXVIII International Symposium on Lattice Field Theory — PoS(Lattice 2010) | 2011
Richard Galvez; Simon Catterall
= 4 supersymmetric Yang-Mills theory.
arXiv: High Energy Physics - Lattice | 2011
Dhagash Mehta; Simon Catterall; Anosh Joseph; Richard Galvez
Within the minimal supersymmetric Standard Model (MSSM), LHC bounds suggest that scalar superpartner masses are far above the electroweak scale. Given a high superpartner mass, nonthermal dark matter is a viable alternative to WIMP dark matter generated via freezeout. In the presence of moduli fields, nonthermal dark matter production is associated with a long matter-dominated phase, modifying the spectral index and primordial tensor amplitude relative to those in a thermalized primordial universe. Nonthermal dark matter can have a higher self-interaction cross section than its thermal counterpart, enhancing astrophysical bounds on its annihilation signals. We constrain the contributions to the neutralino mass from the bino, wino and Higgsino using existing astrophysical bounds and direct detection experiments for models with nonthermal neutralino dark matter. Using these constraints we quantify the expected change to inflationary observables resulting from the nonthermal phase.
arXiv: High Energy Physics - Lattice | 2012
Richard Galvez; Simon Catterall; Dhagash Mehta; Anosh Joseph
A bstractWe make a first study of the phase diagram of four-dimensional
Archive | 2011
Richard Galvez; Simon Catterall; Anosh Joseph; Dhagash Mehta
\mathcal{N}=4