745 research outputs found
#dssf16+1: Library-led Digital Scholarship for Undergraduates at a Small Institution
Librarian R.C. Miessler and Digital Scholarship Fellows Keira Koch, Julia Wall, and Lauren White were invited to speak to at the Pennsylvania Library Association, College and Research Division, Spring Conference about their experiences with the first cohort of the Digital Scholarship Summer Fellowship
#dssf16: Library-led Digital Scholarship for Undergraduates at a Small Institution
In the summer of 2016, Gettysburg Collegeâs Musselman Library piloted the Digital Scholarship Summer Fellowship (DSSF), a library-led, student-centered introduction to digital scholarship. The Fellowship, a 10-week, paid, summer program for rising sophomores and juniors, is programmatic, based on a curriculum designed to introduce the student fellows to digital tools, project management, documentation, and the philosophy behind digital scholarship. The Fellowship aimed to create a digital scholarship community of practice at Gettysburg College, collaborating with educational technologists and faculty engaged in digital scholarship to support the needs of the first cohort; in addition, the Fellowship supported the digital scholarship activities of students participating in other summer research programs. R.C. Miessler, coordinator of the Digital Scholarship Summer Fellowship, will discuss the creation, development, implementation, and future of the program. The student fellows, Keira Koch, Julia Wall, and Lauren White, will reflect on their experience and present the digital projects they created
Giant Gravitons - with Strings Attached (III)
We develop techniques to compute the one-loop anomalous dimensions of
operators in the super Yang-Mills theory that are dual to open
strings ending on boundstates of sphere giant gravitons. Our results, which are
applicable to excitations involving an arbitrary number of open strings,
generalize the single string results of hep-th/0701067. The open strings we
consider carry angular momentum on an S embedded in the S of the
AdSS background. The problem of computing the one loop anomalous
dimensions is replaced with the problem of diagonalizing an interacting Cuntz
oscillator Hamiltonian. Our Cuntz oscillator dynamics illustrates how the
Chan-Paton factors for open strings propagating on multiple branes can arise
dynamically.Comment: 66 pages; v2: improved presentatio
Coherent photon bremsstrahlung and dynamics of heavy-ion collisions: comparison of different models
Differential spectra of coherent photon bremsstrahlung in relativistic heavy
ion collisions are calculated within various schematic models of the
projectile-target stopping. Two versions of the degradation length model, based
on a phenomenological deceleration law, are considered. The simple shock wave
model is studied analytically. The predictions of these models agree in the
soft photon limit, where the spectrum is determined only by the final velocity
distribution of charged particles. The results of these models in the case of
central Au+Au collisions at various bombarding energies are compared with the
predictions of the microscopic transport model UrQMD. It is shown that at the
AGS energy the coherent photon bremsstrahlung exceeds the photon yield from
-decays at photon energies \omega\loo 50 MeV.Comment: 23 pages RevTeX, 9 eps Figure
Towards a holographic dual of large-N_c QCD
We study N_f D6-brane probes in the supergravity background dual to N_c
D4-branes compactified on a circle with supersymmetry-breaking boundary
conditions. In the limit in which the resulting Kaluza--Klein modes decouple,
the gauge theory reduces to non-supersymmetric, four-dimensional QCD with N_c
colours and N_f << N_c flavours. As expected, this decoupling is not fully
realised within the supergravity/Born--Infeld approximation. For N_f = 1 and
massless quarks, m_q = 0, we exhibit spontaneous chiral symmetry breaking by a
quark condensate, \neq 0, and find the associated massless
`pion' in the spectrum. The latter becomes massive for m_q > 0, obeying the
Gell-Mann--Oakes--Renner relation: M_pi^2= - m_q / \f_pi^2. In
the case N_f > 1 we provide a holographic version of the Vafa--Witten theorem,
which states that the U(N_f) flavour symmetry cannot be spontaneously broken.
Further we find N_f^2 - 1 unexpectedly light pseudo-scalar mesons in the
spectrum. We argue that these are not (pseudo) Goldstone bosons and speculate
on the string mechanism responsible for their lightness. We then study the
theory at finite temperature and exhibit a phase transition associated with a
discontinuity in the chiral condensate. D6/anti-D6 pairs are also briefly
discussed.Comment: 43 pages, LaTeX; v3: Scalar vs. pseudo-scalar nature of mesons
clarified, references added. v4: Small change in Acknowledgment
Fluctuating Fuzzy Funnels
It is well known that a D-string ending on a D3, D5 or D7 brane is described
in terms of a non-commutative fuzzy funnel geometry. In this article, we give a
numerical study of the fluctuations about this leading geometry. This allows us
to investigate issues related to the stability and moduli space of these
solutions. We comment on the comparison to the linearized fluctuations in
supergravity.Comment: 24 pages, 3 figures; v2 references added and correcte
Half-BPS Giants, Free Fermions and Microstates of Superstars
We consider 1/2-BPS states in AdS/CFT. Using the matrix model description of
chiral primaries explicit mappings among configurations of fermions, giant
gravitons and the dual-giant gravitons are obtained. These maps lead to a
`duality' between the giant and the dual-giant configurations which is the
reflection of particle-hole duality of the fermion picture. These dualities
give rise to some interesting consequences which we study. We then calculate
the degeneracy of 1/2-BPS states both from the CFT and string theory and show
that they match. The asymptotic degeneracy grows exponentially with the
comformal dimension. We propose that the five-dimensional single charge
`superstar' geometry should carry this density of states. An appropriate
stretched horizon can be placed in this geometry and the entropy predicted by
the CFT and the string theory microstate counting can be reproduced by the
Bekenstein-Hawking formula up to a numerical coefficient. Similar M-theory
examples are also considered.Comment: 21 pages, v2:typos corrected and references adde
Semiclassical Strings, Dipole Deformations of N=1 SYM and Decoupling of KK Modes
In this paper we investigate the recently found -deformed
Maldacena-Nunez background by studying the behavior of different semiclassical
string configurations. This background is conjectured to be dual to dipole
deformations of SYM. We compare our results to those in the pure
Maldacena-Nunez background and show that the energies of our string
configurations are higher than in the undeformed background. Thinking in the
lines of (hep-th/0505100) we argue that this is an evidence for better
decoupling of the Kaluza-Klein modes from the pure SYM theory excitations.
Moreover we are able to find a limit of the background in which the string
energy is independent of , these strings are interpreted as
corresponding to pure gauge theory effects.Comment: 31 pages, references added, new solutions in Section 7 presented, an
appendix added, to appear in JHE
Entropy of near-extremal black holes in AdS_5
We construct the microstates of near-extremal black holes in AdS_5 x S^5 as
gases of defects distributed in heavy BPS operators in the dual SU(N)
Yang-Mills theory. These defects describe open strings on spherical D3-branes
in the S^5, and we show that they dominate the entropy by directly enumerating
them and comparing the results with a partition sum calculation. We display new
decoupling limits in which the field theory of the lightest open strings on the
D-branes becomes dual to a near-horizon region of the black hole geometry. In
the single-charge black hole we find evidence for an infrared duality between
SU(N) Yang-Mills theories that exchanges the rank of the gauge group with an
R-charge. In the two-charge case (where pairs of branes intersect on a line),
the decoupled geometry includes an AdS_3 factor with a two-dimensional CFT
dual. The degeneracy in this CFT accounts for the black hole entropy. In the
three-charge case (where triples of branes intersect at a point), the decoupled
geometry contains an AdS_2 factor. Below a certain critical mass, the
two-charge system displays solutions with naked timelike singularities even
though they do not violate a BPS bound. We suggest a string theoretic
resolution of these singularities.Comment: LaTeX; v2: references and a few additional comments adde
The distribution of transit durations for Kepler planet candidates and implications for their orbital eccentricities
âIn these times, during the rise in the popularity of institutional repositories, the Society does not forbid authors from depositing their work in such repositories. However, the AAS regards the deposit of scholarly work in such repositories to be a decision of the individual scholar, as long as the individual's actions respect the diligence of the journals and their reviewers.â Original article can be found at : http://iopscience.iop.org/ Copyright American Astronomical SocietyDoppler planet searches have discovered that giant planets follow orbits with a wide range of orbital eccentricities, revolutionizing theories of planet formation. The discovery of hundreds of exoplanet candidates by NASA's Kepler mission enables astronomers to characterize the eccentricity distribution of small exoplanets. Measuring the eccentricity of individual planets is only practical in favorable cases that are amenable to complementary techniques (e.g., radial velocities, transit timing variations, occultation photometry). Yet even in the absence of individual eccentricities, it is possible to study the distribution of eccentricities based on the distribution of transit durations (relative to the maximum transit duration for a circular orbit). We analyze the transit duration distribution of Kepler planet candidates. We find that for host stars with T > 5100 K we cannot invert this to infer the eccentricity distribution at this time due to uncertainties and possible systematics in the host star densities. With this limitation in mind, we compare the observed transit duration distribution with models to rule out extreme distributions. If we assume a Rayleigh eccentricity distribution for Kepler planet candidates, then we find best fits with a mean eccentricity of 0.1-0.25 for host stars with T †5100 K. We compare the transit duration distribution for different subsets of Kepler planet candidates and discuss tentative trends with planetary radius and multiplicity. High-precision spectroscopic follow-up observations for a large sample of host stars will be required to confirm which trends are real and which are the results of systematic errors in stellar radii. Finally, we identify planet candidates that must be eccentric or have a significantly underestimated stellar radius.Peer reviewedFinal Accepted Versio
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