3,773 research outputs found
LHCb status and charm physics program
LHCb is a dedicated flavor physics experiment that will observe the 14 TeV
proton-proton collisions at CERN's Large Hadron Collider (LHC). Construction of
the LHCb detector is near completion, commissioning of the detector is well
underway, and LHCb will be fully operational and ready to take data in advance
of the projected May 2008 turn-on date for the LHC. The LHCb software trigger
will feature a dedicated channel for events containing D* mesons that will
dramatically enhance the statistical reach of LHCb in many charm physics
measurements. The LHCb charm physics program is initially focused on mixing and
CP violation measurements in two body decay modes of D0. A much broader program
is possible and will be explored as manpower allows. We intend to use both
promptly produced charm and secondary charm from B meson decays in
measurements. Initial studies have focused on using secondary D*+ mesons for
mixing measurements in two body decays. Preliminary Monte Carlo studies
indicate that LHCb may obtain a statistical precision of \sigma(x'^2) = +/-
0.064 x 10^{-3} (stat) and \sigma(y') = +/- 0.87 x 10^{-3} (stat) from a time
dependent mixing analysis of wrong sign two body D0 --> pi- K+ decays and a
statistical precision of \sigma(y_{CP}) = +/- 0.5 x 10^{-3} (stat) from a ratio
of the lifetimes of D0 decays to the final states K- K+ and K- pi+ in 10
fb^{-1} of data.Comment: To be published in the proceedings of CHARM07, Ithaca, NY, August
2007, eConf C070805. Updated to respect collaboration authorship convention
Dense Quarks, and the Fermion Sign Problem, in a SU(N) Matrix Model
We study the effect of dense quarks in a SU(N) matrix model of deconfinement.
For three or more colors, the quark contribution to the loop potential is
complex. After adding the charge conjugate loop, the measure of the matrix
integral is real, but not positive definite. In a matrix model, quarks act like
a background Z(N) field; at nonzero density, the background field also has an
imaginary part, proportional to the imaginary part of the loop. Consequently,
while the expectation values of the loop and its complex conjugate are both
real, they are not equal. These results suggest a possible approach to the
fermion sign problem in lattice QCD.Comment: 9 pages, 3 figure
Degravitation, Inflation and the Cosmological Constant as an Afterglow
In this report, we adopt the phenomenological approach of taking the
degravitation paradigm seriously as a consistent modification of gravity in the
IR, and investigate its consequences for various cosmological situations. We
motivate degravitation-- where Netwon's constant is promoted to a scale
dependent filter function-- as arising from either a small (resonant) mass for
the graviton, or as an effect in semi-classical gravity. After addressing how
the Bianchi identities are to be satisfied in such a set up, we turn our
attention towards the cosmological consequences of degravitation. By
considering the example filter function corresponding to a resonantly massive
graviton (with a filter scale larger than the present horizon scale), we show
that slow roll inflation, hybrid inflation and old inflation remain
quantitatively unchanged. We also find that the degravitation mechanism
inherits a memory of past energy densities in the present epoch in such a way
that is likely significant for present cosmological evolution. For example, if
the universe underwent inflation in the past due to it having tunneled out of
some false vacuum, we find that degravitation implies a remnant `afterglow'
cosmological constant, whose scale immediately afterwards is parametrically
suppressed by the filter scale () in Planck units . We discuss circumstances through which this scenario reasonably
yields the presently observed value for . We also
find that in a universe still currently trapped in some false vacuum state,
resonance graviton models of degravitation only degravitate initially Planck or
GUT scale energy densities down to the presently observed value over timescales
comparable to the filter scale.Comment: To appear in JCAP; sections discussing degravitation as a
semi-classical effect and the modified Bianchi identities adde
Dressing the Giant Magnon II
We extend our earlier work by demonstrating how to construct classical string
solutions describing arbitrary superpositions of scattering and bound states of
dyonic giant magnons on S^5 using the dressing method for the SU(4)/Sp(2) coset
model. We present a particular scattering solution which generalizes solutions
found in hep-th/0607009 and hep-th/0607044 to the case of arbitrary magnon
momenta. We compute the classical time delay for the scattering of two dyonic
magnons carrying angular momenta with arbitrary relative orientation on the
S^5.Comment: 13 pages, harvma
Shared mission operations concept
Historically, new JPL flight projects have developed a Mission Operations System (MOS) as unique as their spacecraft, and have utilized a mission-dedicated staff to monitor and control the spacecraft through the MOS. NASA budgetary pressures to reduce mission operations costs have led to the development and reliance on multimission ground system capabilities. The use of these multimission capabilities has not eliminated an ongoing requirement for a nucleus of personnel familiar with a given spacecraft and its mission to perform mission-dedicated operations. The high cost of skilled personnel required to support projects with diverse mission objectives has the potential for significant reduction through shared mission operations among mission-compatible projects. Shared mission operations are feasible if: (1) the missions do not conflict with one another in terms of peak activity periods, (2) a unique MOS is not required, and (3) there is sufficient similarity in the mission profiles so that greatly different skills would not be required to support each mission. This paper will further develop this shared mission operations concept. We will illustrate how a Discovery-class mission would enter a 'partner' relationship with the Voyager Project, and can minimize MOS development and operations costs by early and careful consideration of mission operations requirements
Orientifolded Locally AdS3 Geometries
Continuing the analysis of [arXiv:1003.4089[hep-th]], we classify all locally
AdS3 stationary axi-symmetric unorientable solutions to AdS3 Einstein gravity
and show that they are obtained by applying certain orientifold projection on
AdS3, BTZ or AdS3 self-dual orbifold, respectively O-AdS3, O-BTZ and O-SDO
geometries. Depending on the orientifold fixed surface, the O-surface, which is
either a space-like 2D plane or cylinder, or a light-like 2D plane or cylinder
one can distinguish four distinct cases. For the space-like orientifold plane
or cylinder cases these geometries solve AdS3 Einstein equations and are hence
locally AdS3 everywhere except at the O-surface, where there is a
delta-function source. For the light-like cases the geometry is a solution to
Einstein equations even at the O-surface. We discuss the causal structure for
static, extremal and general rotating O-BTZ and O-SDO cases as well as the
geodesic motion on these geometries. We also discuss orientifolding Poincare
patch AdS3 and AdS2 geometries as a way to geodesic completion of these spaces
and comment on the 2D CFT dual to the O-geometries.Comment: 26 page, 4 .eps figure
Tachyons in de Sitter space and analytical continuation from dS/CFT to AdS/CFT
We discuss analytic continuation from d-dimensional Lorentzian de Sitter
(dS) to d-dimensional Lorentzian anti-de Sitter (AdS) spacetime. We
show that AdS, with opposite signature of the metric, can be obtained as
analytic continuation of a portion of dS. This implies that the dynamics of
(positive square-mass) scalar particles in AdS can be obtained from the
dynamics of tachyons in dS. We discuss this correspondence both at the
level of the solution of the field equations and of the Green functions. The
AdS/CFT duality is obtained as analytic continuation of the dS/CFT duality.Comment: 17 pages, 1 figure, JHEP styl
Quantum Entropy Function from AdS(2)/CFT(1) Correspondence
We review and extend recent attempts to find a precise relation between
extremal black hole entropy and degeneracy of microstates using AdS_2/CFT_1
correspondence. Our analysis leads to a specific relation between degeneracy of
black hole microstates and an appropriately defined partition function of
string theory on the near horizon geometry, -- named the quantum entropy
function. In the classical limit this reduces to the usual relation between
statistical entropy and Wald entropy.Comment: LaTeX file, 27 pages, A modified and extended version of the talk
given at Strings 200
PP-wave and Non-supersymmetric Gauge Theory
We extend the pp-wave correspondence to a non supersymmetric example. The
model is the type 0B string theory on the pp-wave R-R background. We explicitly
solve the model and give the spectrum of physical states. The field theory
counterpart is given by a sector of the large N SU(N) x SU(N) CFT living on a
stack of N electric and N magnetic D3-branes. The relevant effective coupling
constant is g_{eff}=g_sN/J^2. The string theory has a tachyon in the spectrum,
whose light-cone energy can be exactly computed as a function of g_{eff}. We
argue that the perturbative analysis in g_{eff} in the dual gauge theory is
reliable, with corrections of non perturbative type. We find a precise
state/operator map, showing that the first perturbative corrections to the
anomalous dimensions of the operators have the behavior expected from the
string analysis.Comment: 19 pages. Revised versio
Giant Magnons and Singular Curves
We obtain the giant magnon of Hofman-Maldacena and its dyonic generalisation
on R x S^3 < AdS_5 x S^5 from the general elliptic finite-gap solution by
degenerating its elliptic spectral curve into a singular curve. This alternate
description of giant magnons as finite-gap solutions associated to singular
curves is related through a symplectic transformation to their already
established description in terms of condensate cuts developed in
hep-th/0606145.Comment: 34 pages, 17 figures, minor change in abstrac
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