1,055 research outputs found
Cross Section Measurements of Hard Diffraction at the SPS-Collider
The UA8 experiment previously reported the observation of jets in diffractive
events containing leading protons (``hard diffraction''), which was interpreted
as evidence for the partonic structure of an exchanged Reggeon, believed to be
the Pomeron . In the present Letter, we report the final UA8 hard-diffractive
(jet) cross section results and their interpretation. After corrections, the
fraction of single diffractive events with mass from 118 to 189 GeV that have
two scattered partons, each with Et_jet > 8 GeV, is in the range 0.002 to 0.003
(depending on x_p). We determine the product, fK, of the fraction by which the
Pomeron's momentum sum rule is violated and the normalization constant of the
Pomeron-Flux-Factor of the proton. For a pure gluonic- or a pure qqbar-Pomeron
, respectively: fK = 0.30 +- 0.05 +- 0.09) and (0.56 +- 0.09 +- 0.17) GeV^-2.Comment: 20 pages, 5 Encapsulated Postscript figures, LaTex, Final Version,
Physics Letters B (in Pess 1998
A Study of Inclusive Double-Pomeron-Exchange in p pbar -> p X pbar at root s = 630 GeV
We report measurements of the inclusive reaction, p pbar -> p X pbar, in
events where either or both the beam-like final-state baryons were detected in
Roman-pot spectrometers and the central system was detected in the UA2
calorimeter. A Double-Pomeron-Exchange (DPE) analysis of these data and single
diffractive data from the same experiment demonstrates that, for central masses
of a few GeV, the extracted Pomeron-Pomeron total cross section exhibits an
enhancement which exceeds factorization expectations by an order-of-magnitude.
This may be a signature for glueball production. The enhancement is shown to be
independent of uncertainties connected with possible non-universality of the
Pomeron flux factor. Based on our analysis, we present DPE cross section
predictions, for unit (1 mb) Pomeron-Pomeron total cross section, at the
Tevatron, LHC and the 920 GeV fixed-target experiment, HERA-B.Comment: 52 pages, 27 Encapsulated Postscript figures, 3 Tables, LaTex,
Revised version as it will appear in European Physics Journal
Methods for Reducing False Alarms in Searches for Compact Binary Coalescences in LIGO Data
The LIGO detectors are sensitive to a variety of noise transients of
non-astrophysical origin. Instrumental glitches and environmental disturbances
increase the false alarm rate in the searches for gravitational waves. Using
times already identified when the interferometers produced data of questionable
quality, or when the channels that monitor the interferometer indicated
non-stationarity, we have developed techniques to safely and effectively veto
false triggers from the compact binary coalescences (CBCs) search pipeline
First search for gravitational waves from the youngest known neutron star
We present a search for periodic gravitational waves from the neutron star in the supernova remnant Cassiopeia
A. The search coherently analyzes data in a 12 day interval taken from the fifth science run of the Laser
Interferometer Gravitational-Wave Observatory. It searches gravitational-wave frequencies from 100 to 300 Hz
and covers a wide range of first and second frequency derivatives appropriate for the age of the remnant and
for different spin-down mechanisms. No gravitational-wave signal was detected. Within the range of search
frequencies, we set 95% confidence upper limits of (0.7â1.2) Ă 10^(â24) on the intrinsic gravitational-wave
strain, (0.4â4) Ă 10^(â4) on the equatorial ellipticity of the neutron star, and 0.005â0.14 on the amplitude of
r-mode oscillations of the neutron star. These direct upper limits beat indirect limits derived from energy
conservation and enter the range of theoretical predictions involving crystalline exotic matter or runaway r-modes.
This paper is also the first gravitational-wave search to present upper limits on the r-mode amplitude
Search for Gravitational-wave Inspiral Signals Associated with Short Gamma-ray Bursts During LIGO's Fifth and Virgo's First Science Run
Progenitor scenarios for short gamma-ray bursts (short GRBs) include coalescenses of two neutron stars or a neutron star and black hole, which would necessarily be accompanied by the emission of strong gravitational waves. We present a search for these known gravitational-wave signatures in temporal and directional coincidence with 22 GRBs that had sufficient gravitational-wave data available in multiple instruments during LIGO's fifth science run, S5, and Virgo's first science run, VSR1. We find no statistically significant gravitational-wave candidates within a [ â 5, + 1) s window around the trigger time of any GRB. Using the Wilcoxon-Mann-Whitney U-test, we find no evidence for an excess of weak gravitational-wave signals in our sample of GRBs. We exclude neutron star-black hole progenitors to a median 90% confidence exclusion distance of 6.7 Mpc
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