4,716 research outputs found
New Signatures of Squarks
When the gluino is light and long lived, missing energy is a poor signature
for both squarks and gluinos. Instead, production in and
collisions characteristically results in events with jets.
Methods are proposed for deciding whether an observed excess of 4-jet events is
due to production. The recent report by ALEPH of observation of 14
4-jet events when 7 were expected is discussed.Comment: 12/22/95 version (put on net 1/1/96) elaborates remarks on squarks as
possible source of ALEPH 4-jet excess and adds a ref. latex, 10 pages
(including 1 figure), uufile
Neutron Stars with a Stable, Light Supersymmetric Baryon
If a light gluino exists, the lightest gluino-containing baryon, the \OSO, is
a possible candidate for self-interacting dark matter. In this scenario, the
simplest explanation for the observed ratio
is that \MeVcs; this is not at present excluded by particle
physics. Such an \OSO could be present in neutron stars, with hyperon formation
serving as an intermediate stage. We calculate equilibrium compositions and
equation of state for high density matter with the \OSO, and find that for a
wide range of parameters the properties of neutron stars with the \OSO are
consistent with observations. In particular, the maximum mass of a nonrotating
star is , and the presence of the \OSO is helpful in
reconciling observed cooling rates with hyperon formation.Comment: ApJL submitted, 4 pages, using emulateapj (very very minor changes to
match published versio
Hamara Healthy Living Centre - an evaluation
Hamara is a Healthy Living Centre which aims to improve health and well-being through providing a range of culturally appropriate activities and services. Hamara has a vision of 'bringing communities together' and since it was established in 2004, the Centre has provided a valuable community resource in South Leeds. Partnership work between Hamara and Leeds Met goes back to 2002. In 2007, the Centre for Health Promotion Research carried out an evaluation of Hamara in partnership with Hamara staff and Leeds Met Community Partnerships and Volunteering. This was followed by a highly successful community cohesion conference 'One Community' which was held at Hamara on 10th October 2008, and was supported through a Leeds Met public engagement grant. The event attracted over a hundred people from diverse communities and organisations across Leeds. A packed audience heard Hilary Benn, local MP and Patron of Hamara, talk about the importance of working in collaboration around community cohesion. Jane South, Centre for Health Promotion Research, presented the main evaluation results and set out the some challenges for the future. The proceedings concluded with the presentation of awards to a number of for local community champions who work to bring people together and make a real difference in the city of Leeds
Where do "red and dead" early-type void galaxies come from?
Void regions of the Universe offer a special environment for studying
cosmology and galaxy formation, which may expose weaknesses in our
understanding of these phenomena. Although galaxies in voids are observed to be
predominately gas rich, star forming and blue, a sub-population of bright red
void galaxies can also be found, whose star formation was shut down long ago.
Are the same processes that quench star formation in denser regions of the
Universe also at work in voids?
We compare the luminosity function of void galaxies in the 2dF Galaxy
Redshift Survey, to those from a galaxy formation model built on the Millennium
Simulation. We show that a global star formation suppression mechanism in the
form of low luminosity "radio mode" AGN heating is sufficient to reproduce the
observed population of void early-types. Radio mode heating is environment
independent other than its dependence on dark matter halo mass, where, above a
critical mass threshold of approximately M_vir~10^12.5 M_sun, gas cooling onto
the galaxy is suppressed and star formation subsequently fades. In the
Millennium Simulation, the void halo mass function is shifted with respect to
denser environments, but still maintains a high mass tail above this critical
threshold. In such void halos, radio mode heating remains efficient and red
galaxies are found; collectively these galaxies match the observed space
density without any modification to the model. Consequently, galaxies living in
vastly different large-scale environments but hosted by halos of similar mass
are predicted to have similar properties, consistent with observations.Comment: 6 pages, 3 figures, accepted MNRA
Charmonium Suppression - Interplay of Hadronic and Partonic Degrees of Freedom
Last year the E866-group of the Fermilab measured the dependence of
and suppression in collisions. We discuss two of the
effects found in that experiment with regard to color coherence effects: the
different suppression of the and the at and the
significant suppression of both at large . The small regions is
dominated by fully formed charmonium states and thus enables us to discuss the
formation time and the cross section of the different charmonium states. In the
large region the interaction of the charmonium states with nuclear matter
has to be described by partonic degrees of freedom, because in that kinematic
domain the formation time is much larger than the nuclear radii. The
understanding of this region will be crucial for the interpretation of the data
of the future heavy ion colliders RHIC and LHC.Comment: 4 pages, 1 table, 1 figure, Contribution to the Proceedings of the
15th Particles and Nuclei International Conference (PANIC 99), Uppsala,
Sweden, June 10-16, 199
Cosmic Ray Spallation in Radio-Quiet Active Galactic Nuclei: A Case Study of NGC 4051
We investigate conditions for and consequences of spallation in radio-quiet
Seyfert galaxies. The work is motivated by the recent discovery of significant
line emission at 5.44 keV in Suzaku data from NGC 4051. The energy of the new
line suggests an identification as Cr I Ka emission, however the line is much
stronger than would be expected from material with cosmic abundances, leading
to a suggestion of enhancement owing to nuclear spallation of Fe by low energy
cosmic rays from the active nucleus. We find that the highest abundance
enhancements are likely to take place in gas out of the plane of the accretion
disk and that timescales for spallation could be as short as a few years. The
suggestion of a strong nuclear flux of cosmic rays in a radio-quiet Seyfert
galaxy is of particular interest in light of the recent suggestion from Pierre
Auger Observatory data that ultra-high-energy cosmic rays may originate in such
sources.Comment: 14 pages, 1 figure. Accepted for publication in The Astrophysical
Journa
Experiments to Find or Exclude a Long-Lived, Light Gluino
Gluinos in the mass range ~1 1/2 - 3 1/2 GeV are absolutely excluded. Lighter
gluinos are allowed, except for certain ranges of lifetime. Only small parts of
the mass-lifetime parameter space are excluded for larger masses unless the
lifetime is shorter than ~ 2 10^{-11} (m_{gluino}/ GeV) sec. Refined mass and
lifetime estimates for R-hadrons are given, present direct and indirect
experimental constraints are reviewed, and experiments to find or definitively
exclude these possibilities are suggested.Comment: 27 pp, latex with 1 uufiled figure, RU-94-35. New version amplifies
discussion of some points and corresponds to version for Phys. Rev.
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