Haim Goldberg
Northeastern University
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Featured researches published by Haim Goldberg.
Physical Review D | 2002
Luis A. Anchordoqui; Jonathan L. Feng; Haim Goldberg; Alfred D. Shapere
If extra spacetime dimensions and low-scale gravity exist, black holes will be produced in observable collisions of elementary particles. For the next several years, ultrahigh-energy cosmic rays provide the most promising window on this phenomenon. In particular, cosmic neutrinos can produce black holes deep in the Earths atmosphere, leading to quasihorizontal giant air showers. We determine the sensitivity of cosmic ray detectors to black hole production and compare the results to other probes of extra dimensions. With
Physical Review Letters | 2008
Luis A. Anchordoqui; Haim Goldberg; Dieter Lüst; Satoshi Nawata; Stephan Stieberger; Tomasz R. Taylor
ng~4
Physical Review D | 2002
Luis A. Anchordoqui; Haim Goldberg
extra dimensions, current bounds on deeply penetrating showers from AGASA already provide the most stringent bound on low-scale gravity, requiring a fundamental Planck scale
Journal of High Energy Astrophysics | 2014
Luis A. Anchordoqui; V. Barger; Ilias Cholis; Haim Goldberg; Dan Hooper; Alexander Kusenko; J. G. Learned; Danny Marfatia; Sandip Pakvasa; Thomas C. Paul; Thomas Weiler
{M}_{D}g1.3\char21{}1.8 \mathrm{TeV}.
Nuclear Physics | 2009
Luis A. Anchordoqui; Tomasz R. Taylor; Satoshi Nawata; Stephan Stieberger; Haim Goldberg; Dieter Lust
The Auger Observatory will probe
Physical Review D | 2002
Luis A. Anchordoqui; Jonathan L. Feng; Haim Goldberg; Alfred D. Shapere
{M}_{D}
Physics Letters B | 1986
Haim Goldberg; Lawrence J. Hall
as large as 4 TeV and may observe on the order of a hundred black holes in 5 years. We also consider the implications of angular momentum and possible exponentially suppressed parton cross sections; including these effects, large black hole rates are still possible. Finally, we demonstrate that even if only a few black hole events are observed, a standard model interpretation may be excluded by comparison with Earth-skimming neutrino rates.
Physics Letters B | 1987
Hideaki Aoyama; Haim Goldberg
Assuming that the fundamental string mass scale is in the TeV range and the theory is weakly coupled, we discuss possible signals of string physics at the Large Hadron Collider (LHC). In D-brane constructions, the dominant contributions to full-fledged string amplitudes for all the common QCD parton subprocesses leading to dijets are completely independent of the details of compactification, and can be evaluated in a parameter-free manner. We make use of these amplitudes evaluated near the first resonant pole to determine the discovery potential of LHC for the first Regge excitations of the quark and gluon. Remarkably, the reach of LHC after a few years of running can be as high as 6.8 TeV. Even after the first 100 pb(-1) of integrated luminosity, string scales as high as 4.0 TeV can be discovered. Data on pp-->directgamma + jet can provide corroboration for string physics at scales as high as 5 TeV.
Physics Letters B | 2016
Luis A. Anchordoqui; Ignatios Antoniadis; Haim Goldberg; Xing Huang; Dieter Lüst; Tomasz R. Taylor
The existence of extra degrees of freedom beyond the electroweak scale may allow the formation of black holes in nearly horizontal neutrino air showers. In this paper we examine the average properties of the light descendants of these black holes. Our analysis indicates that black hole decay gives rise to deeply penetrating showers with an electromagnetic component which differs substantially from that in conventional neutrino interactions, allowing a good characterization of the phenomenon against background. Naturally occurring black holes in horizontal neutrino showers could be detected and studied with the Auger air shower array. Since the expected black hole production rate at Auger is
Physics Letters B | 1990
Haim Goldberg
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