Sanghyeon Chang
University of Florida
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Featured researches published by Sanghyeon Chang.
Nuclear Physics | 1996
Sanghyeon Chang; Claudio Coriano; Alon E. Faraggi
We investigate the cosmological constraints on exotic stable matter states which arise in realistic free fermionic superstring models. These states appear in the superstring models due to a “Wilsonline” breaking of the unifying non-abelian gauge symmetry. In the models that we consider the unifying SO(10) gauge symmetry is broken at the string level to SO(6) x SO(4), SU(5) x U(1) or SU(3) x SU(2) x U(1)2. The exotic matter states are classified according to the patterns of the SO(10) symmetry breaking. In SO(6) x SO(4) and SU(5) x U(1) type models one obtains fractionally charged states with Qe.m. = ±12. In SU (3) x SU (2) x U(1)2 type models one also obtains states with the regular charges under the Standard Model gauge group but with “fractional” charges under the U(1)z′ symmetry. These states include down-like color triplets and electroweak doublets, as well as states which are Standard Model singlets. By analyzing the renormalizable and nonrenormalizable terms of the superpotential in a specific superstring model, we show that these exotic states can be stable. We investigate the cosmological constraints on the masses and relic density of the exotic states. We propose that, while the abundance and the masses of the fractionally charged states are highly constrained, the Standard Model-like states, and in particular the Standard Model singlet, are good dark matter candidates.
Physical Review D | 1998
Sanghyeon Chang; C. Hagmann; P. Sikivie
We discuss the appearance at the QCD phase transition, and the subsequent decay, of axion walls bounded by strings in
Physical Review Letters | 1996
Sanghyeon Chang; Hang Bae Kim
N=1
Nuclear Physics | 1998
Sanghyeon Chang; Claudio Coriano; R. D. Field; L. E. Gordon
axion models. We argue on intuitive grounds that the main decay mechanism is into barely relativistic axions. We present numerical simulations of the decay process. In these simulations, the decay happens immediately, in a time scale of order the light travel time, and the average energy of the radiated axions is
arXiv: High Energy Physics - Phenomenology | 1999
C. Hagmann; Sanghyeon Chang; P. Sikivie
〈{\ensuremath{\omega}}_{a}〉\ensuremath{\simeq}{7m}_{a}
Nuclear Physics | 1998
Sanghyeon Chang; Claudio Coriano; R. D. Field
for
Physical Review D | 2012
Sanghyeon Chang; Kang Young Lee; So Young Shim; Jeonghyeon Song
{v}_{a}{/m}_{a}\ensuremath{\simeq}500.
Physical Review D | 1998
Sanghyeon Chang; Claudio Coriano; L. E. Gordon
arXiv: High Energy Physics - Phenomenology | 1999
Sanghyeon Chang; C. Hagmann; P. Sikivie
〈{\ensuremath{\omega}}_{a}〉
Physical Review D | 1994
Sanghyeon Chang; Jihn E. Kim
is found to increase approximately linearly with