35 research outputs found
Identification of high energy gamma-ray sources and source populations in the era of deep all-sky coverage
A large fraction of the anticipated source detections by the Gamma-ray Large
Area Space Telescope (GLAST-LAT) will initially be unidentified. We argue that
traditional approaches to identify individuals and/or populations of gamma ray
sources will encounter procedural limitations. Those limitations are discussed
on the background of source identifications from EGRET observations. Generally,
our ability to classify (faint) source populations in the anticipated GLAST
dataset with the required degree of statistical confidence will be hampered by
sheer source wealth. A new paradigm for achieving the classification of gamma
ray source populations is discussed.Comment: Comments: 6 pages, 2 figures, Accepted for publication in
Astrophysics and Space Science, Proc. of "The Multi-Messenger Approach to
High-Energy Gamma-ray Sources (Third Workshop on the Nature of Unidentified
High-Energy Sources)", Barcelona, July 4-7, 200
A New Upper Limit for the Tau-Neutrino Magnetic Moment
Using a prompt neutrino beam in which a nu_tau component was identified for
the first time, the nu_tau magnetic moment was measured based on a search for
an anomalous increase in the number of neutrino-electron interactions. One such
event was observed when 2.3 were expected from background processes, giving an
upper 90% confidence limit of 3.9x10^-7 Bohr magnetons.Comment: 9 pages; 1 figur
Microlensing as a probe of the Galactic structure; 20 years of microlensing optical depth studies
Microlensing is now a very popular observational astronomical technique. The
investigations accessible through this effect range from the dark matter
problem to the search for extra-solar planets. In this review, the techniques
to search for microlensing effects and to determine optical depths through the
monitoring of large samples of stars will be described. The consequences of the
published results on the knowledge of the Milky-Way structure and its dark
matter component will be discussed. The difficulties and limitations of the
ongoing programs and the perspectives of the microlensing optical depth
technique as a probe of the Galaxy structure will also be detailed.Comment: Accepted for publication in General Relativity and Gravitation.
General Relativity and Gravitation in press (2010) 0
Search for Rare and Forbidden Dilepton Decays of the D+, Ds, and D0 Charmed Mesons
We report the results of a search for flavor-changing neutral current,
lepton-flavor violating, and lepton-number violating decays of D+, Ds, and D0
mesons (and their antiparticles) into modes containing muons and electrons.
Using data from Fermilab charm hadroproduction experiment E791, we examine the
pi,l,l and K,l,l decay modes of D+ and Ds and the l+l- decay modes of D0. No
evidence for any of these decays is found. Therefore, we present
branching-fraction upper limits at 90% confidence level for the 24 decay modes
examined. Eight of these modes have no previously reported limits, and fourteen
are reported with significant improvements over previously published results.Comment: 12 pages, 3 figures, LaTeX, elsart.cls, epsf.sty, amsmath.sty
Submitted to Physics Letters