21,329 research outputs found
Very High Energy Gamma Rays from Supernova Remnants and Constraints on the Galactic Interstellar Radiation Field
The large-scale Galactic interstellar radiation field (ISRF) is the result of
stellar emission and dust re-processing of starlight. Where the energy density
of the ISRF is high (e.g., the Galactic Centre), the dominant gamma-ray
emission in individual supernova remnants (SNRs), such as G0.9+0.1, may come
from inverse Compton (IC) scattering of the ISRF. Several models of the ISRF
exist. The most recent one, which has been calculated by us, predicts a
significantly higher ISRF than the well-used model of Mathis, Mezger, and
Panagia. However,comparison with data is limited to local observations. Based
on our current estimate of the ISRF we predict the gamma-ray emission in the
SNRs G0.9+0.1 and RXJ1713, and pair-production absorption features above 20 TeV
in the spectra of G0.9+0.1, J1713-381, and J1634-472. We discuss how GLAST,
along with current and future very high energy instruments, may be able to
provide upper bounds on the large-scale ISRF.Comment: To appear in the proceedings of the 1st GLAST Symposiu
A Comprehensive Four-Quark Interpretation of D_s(2317), D_s(2457) and D_s(2632)
The recently observed new member of the charm-strange family D_s(2632) which
has a surprisingly narrow width is challenging our theory. D_s(2317) and
D_s(2457) which were observed earlier have similar behaviors and receive
various theoretical explanations. Some authors use the heavy hadron chiral
effective theory to evaluate heavy-light quark systems and obtain a reasonable
evaluation on the masses of D_s(2317) and D_s(2457). An alternative picture is
to interpret them as four-quark or molecular states. In this work, we are
following the later and propose a unitive description for all the three new
members D_s(2632), D_s(2317) and D_s(2457) and at least, so far our picture is
consistent with the data.Comment: 6 page
Hadronic Gamma Rays from Supernova Remnants
A gas cloud near a supernova remnant (SNR) provides a target for
pp-collisions leading to subsequent gamma-ray emission through neutral pion
decay. The assumption of a power-law ambient spectrum of accelerated particles
with index near -2 is usually built into models predicting the spectra of
very-high energy (VHE) gamma-ray emission from SNRs. However, if the gas cloud
is located at some distance from the SNR shock, this assumption is not
necessarily correct. In this case, the particles which interact with the cloud
are those leaking from the shock and their spectrum is approximately
monoenergetic with the injection energy gradually decreasing as the SNR ages.
In the GLAST energy range the gamma-ray spectrum resulting from particle
interactions with the gas cloud will be flatter than expected, with the cutoff
defined by the pion momentum distribution in the laboratory frame. We evaluate
the flux of particles escaping from a SNR shock and apply the results to the
VHE diffuse emission detected by the HESS at the Galactic centre.Comment: 4 pages, 3 figures. Contribution to the 30th ICRC, Merida, Mexico,
2007 (final version
Between the classroom and the field: An examination of the experiences of black male football student-athletes
This study is concerned with the fact that numerous Black student-athletes that play football at Division 1 predominantly White institutions (PWIs) are graduating at the lowest rates of all student and student-athlete groups on college campuses nationwide. An intercollegiate athletics system acts as the commercial arm of the university and is designed to ensure the sustainability and viability of football by creating contradictory athletic and academic pressures that the student-athletes must navigate. Despite the intentional obstacles that Black student athletes encounter, there are many that do graduate from their institution and transition into a professional career. Therefore, the guiding research question was: How did Black male football student-athletes manage to graduate while being part of a Division 1 team at a research-intensive institution?
Purposeful sampling was used to select participants who met the criteria defined by the researcher. This study utilized a qualitative case study method to examine the experiences of the selected participants. Primary data were collected through interviews from five Black football players and seven current and former university faculty and staff members. Secondary data were collected from participant questionnaires and cross-referenced with media guides and player profiles.
The study revealed three central findings. First, the data disproved the common notion that Black football student-athletes are from inner city, poor socioeconomic backgrounds and attended failing high schools that did not adequately prepare them for college. Second, the participants in this study navigated contradictory athletic and academic pressures when they utilized their strong social support network of people who provided advice, guidance, and a safe space to process feelings. The function of the support was to strengthen their motivation to graduate. Last, the organizational system which these student-athletes had to navigate, influenced all facets of their lives and dictated the degree programs they pursued. The student-athletes that managed to graduate from the institution did so from a degree program that was accommodating to their football related schedules. Implications and suggestions from the author for future research are also discussed
Global Maps of Science based on the new Web-of-Science Categories
In August 2011, Thomson Reuters launched version 5 of the Science and Social
Science Citation Index in the Web of Science (WoS). Among other things, the 222
ISI Subject Categories (SCs) for these two databases in version 4 of WoS were
renamed and extended to 225 WoS Categories (WCs). A new set of 151 Subject
Categories (SCs) was added, but at a higher level of aggregation. Since we
previously used the ISI SCs as the baseline for a global map in Pajek (Rafols
et al., 2010) and brought this facility online (at
http://www.leydesdorff.net/overlaytoolkit), we recalibrated this map for the
new WC categories using the Journal Citation Reports 2010. In the new
installation, the base maps can also be made using VOSviewer (Van Eck &
Waltman, 2010).Comment: Scientometrics, in pres
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