Ali Abbasabadi
Ferris State University
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Featured researches published by Ali Abbasabadi.
Physical Review D | 1998
Ali Abbasabadi; Alberto Devoto; Duane A. Dicus; Wayne W. Repko
A general decomposition of the amplitudes for the 2 {r_arrow} 2 processes {gamma}{nu} {r_arrow} {gamma}{nu} and {gamma}{gamma} {r_arrow} {nu}{bar {nu}} is obtained using gauge invariance and Bose symmetry. The restrictions implied by this decomposition are investigated for the reaction {gamma}{gamma} {r_arrow} {nu}{bar {nu}} by computing the one-loop helicity amplitudes in the standard model. In the center of mass, where {radical}s = 2{omega}, the cross section grows roughly as {omega}{sup 6} up to the threshold for W-boson production, {radical}s = 2m{sub W}. Astrophysical implications of very high energy photon-neutrino interactions are discussed.
Physical Review D | 1998
Ali Abbasabadi; David Bowser-Chao; Duane A. Dicus; Wayne W. Repko
We present cross sections for the reactions p{bar p}{r_arrow}H{gamma} and pp{r_arrow}H{gamma} arising from the subprocess q{bar q}{r_arrow}H{gamma}. The calculation includes the complete one-loop contribution from all light quarks as well as the tree contributions from the light quarks and c and b quarks. These are the main sources of Higgs-photon associated production at hadron colliders. At Fermilab Tevatron energies, the cross section is typically between 0.1thinspfb and 1.0thinspfb for 80thinspGeV{le}m{sub H}{le}160thinspGeV, while at CERN LHC energies it exceeds about 2.0thinspfb over the same range of m{sub H}. While substantial, these cross sections are not large enough to produce a signal which is discernable above the backgrounds from q{bar q}{r_arrow}b{bar b}{gamma} and gg{r_arrow}b{bar b}{gamma}. {copyright} {ital 1998} {ital The American Physical Society}
Physical Review D | 1997
Ali Abbasabadi; D. Bowser-Chao; Duane A. Dicus; Wayne W. Repko
Higgs boson radiative decays of the form
Physical Review D | 2005
Ali Abbasabadi; Wayne W. Repko
H\rightarrow f\bar{f}\gamma
Physical Review D | 2001
Ali Abbasabadi; Alberto Devoto; Wayne W. Repko
are calculated in the Standard Model using the complete one-loop expressions for the decay amplitudes. Contributions to the radiative width from leptons and light quarks are given. We also present
Physical Review D | 2000
Ali Abbasabadi; Wayne W. Repko
e\bar{e}
Journal of High Energy Physics | 2006
Ali Abbasabadi; Wayne W. Repko
invariant mass distributions for
Physical Review D | 1996
Ali Abbasabadi; David Bowser-Chao; Duane A. Dicus; Wayne W. Repko
H\rightarrow e\bar{e}\gamma
Physical Review D | 2003
Ali Abbasabadi; Wayne W. Repko
, which illustrate the importance of the photon pole contribution and the effects of the box diagrams.
Physical Review D | 2001
Ali Abbasabadi; Wayne W. Repko
We have calculated the width of the rare decay H{yields}{gamma}{gamma}Z at one-loop level in the standard model for Higgs boson masses in the range 115 GeV{<=}m{sub H}{<=}160 GeV . For this range of Higgs boson masses we find that Z boson is predominantly longitudinally polarized, and the photons have the same helicity. A comparison of the decay width {gamma}(H{yields}{gamma}{gamma}Z) to those of H{yields}{gamma}{gamma} and H{yields}{gamma}Z shows that, for the Higgs boson mass of m{sub H}{approx}135 GeV, the ratios of the decay widths are {gamma}(H{yields}{gamma}{gamma}Z)/{gamma}(H{yields}{gamma}{gamma}){approx}{gamma}(H{yields}{gamma}{gamma}Z)/{gamma}(H{yields}{gamma}Z){approx}10{sup -5}-10{sup -6}.