869 research outputs found
Confronting QCD Instantons with HERA Data
The sensitivity of existing HERA data on the hadronic final state in
deep-inelastic scattering (DIS) to processes induced by QCD instantons is
systematically investigated. The maximally allowed fraction of such processes
in DIS is found to be on the percent level in the kinematic domain 0.0001 <
x-Bjorken < 0.01 and 5 < Q squared < 100 GeV squared. The best limits are
obtained from the multiplicity distribution.Comment: 5 pages, latex, entire paper w. tex, style and figure
The Dark Matter Annihilation Signal from Galactic Substructure: Predictions for GLAST
We present quantitative predictions for the detectability of individual
Galactic dark matter subhalos in gamma-rays from dark matter pair annihilations
in their centers. Our method is based on a hybrid approach, employing the
highest resolution numerical simulations available (including the recently
completed one billion particle Via Lactea II simulation) as well as analytical
models for the extrapolation beyond the simulations' resolution limit. We
include a self-consistent treatment of subhalo boost factors, motivated by our
numerical results, and a realistic treatment of the expected backgrounds that
individual subhalos must outshine. We show that for reasonable values of the
dark matter particle physics parameters (M_X ~ 50 - 500 GeV and ~
10^-26 - 10^-25 cm^3/s) GLAST may very well discover a few, even up to several
dozen, such subhalos, at 5 sigma significance, and some at more than 20 sigma.
We predict that the majority of luminous sources would be resolved with GLAST's
expected angular resolution. For most observer locations the angular
distribution of detectable subhalos is consistent with a uniform distribution
across the sky. The brightest subhalos tend to be massive (median Vmax of 24
km/s) and therefore likely hosts of dwarf galaxies, but many subhalos with Vmax
as low as 5 km/s are also visible. Typically detectable subhalos are 20 - 40
kpc from the observer, and only a small fraction are closer than 10 kpc. The
total number of observable subhalos has not yet converged in our simulations,
and we estimate that we may be missing up to 3/4 of all detectable subhalos.Comment: 19 pages, 12 figures, ApJ accepted, a version with higher resolution
figures can be downloaded from
http://www.sns.ias.edu/~mqk/transfer/VL2_GLAST_predictions.pd
Formation and evolution of galaxy dark matter halos and their substructure
We use the ``Via Lactea'' simulation to study the co-evolution of a Milky
Way-size LambdaCDM halo and its subhalo population. While most of the host halo
mass is accreted over the first 6 Gyr in a series of major mergers, the
physical mass distribution [not M_vir(z)] remains practically constant since
z=1. The same is true in a large sample of LambdaCDM galaxy halos. Subhalo mass
loss peaks between the turnaround and virialization epochs of a given mass
shell, and declines afterwards. 97% of the z=1 subhalos have a surviving bound
remnant at the present epoch. The retained mass fraction is larger for
initially lighter subhalos: satellites with maximum circular velocities Vmax=10
km/s at z=1 have today about 40% of their mass back then. At the first
pericenter passage a larger average mass fraction is lost than during each
following orbit. Tides remove mass in substructure from the outside in, leading
to higher concentrations compared to field halos of the same mass. This effect,
combined with the earlier formation epoch of the inner satellites, results in
strongly increasing subhalo concentrations towards the Galactic center. We
present individual evolutionary tracks and present-day properties of the likely
hosts of the dwarf satellites around the Milky Way. The formation histories of
``field halos'' that lie today beyond the Via Lactea host are found to strongly
depend on the density of their environment. This is caused by tidal mass loss
that affects many field halos on eccentric orbits.Comment: 20 pages, 18 figures. Figures 6,7 and 8 corrected in this version,
for details see the erratum in ApJ 679, 1680 and
http://www.ucolick.org/~diemand/vl/publ/vlevolerr.pdf. Data, movies and
images are available at http://www.ucolick.org/~diemand/vl
Galactic Substructure and Dark Matter Annihilation in the Milky Way Halo
We study the effects of substructure on the rate of dark-matter annihilation
in the Galactic halo. We use an analytic model for substructure that can extend
numerical simulation results to scales too small to be resolved by the
simulations. We first calibrate the analytic model to numerical simulations,
and then determine the annihilation boost factor, for standard WIMP models as
well as those with Sommerfeld (or other) enhancements, as a function of
Galactocentric radius in the Milky Way. We provide an estimate of the
dependence of the gamma-ray intensity of WIMP annihilation as a function of
angular distance from the Galactic center. This methodology, coupled with
future numerical simulation results can be a powerful tool that can be used to
constrain WIMP properties using Fermi all-sky data.Comment: 10 pages, 7 figures, submitted to Phys. Rev. D; added a few
reference
All-electrical time-resolved spin generation and spin manipulation in n-InGaAs
We demonstrate all-electrical spin generation and subsequent manipulation by
two successive electric field pulses in an n-InGaAs heterostructure in a
time-resolved experiment at zero external magnetic field. The first electric
field pulse along the crystal axis creates a current induced spin
polarization (CISP) which is oriented in the plane of the sample. The
subsequent electric field pulse along [110] generates a perpendicular magnetic
field pulse leading to a coherent precession of this spin polarization with
2-dimensional electrical control over the final spin orientation. Spin
precession is probed by time-resolved Faraday rotation. We determine the
build-up time of CISP during the first field pulse and extract the spin
dephasing time and internal magnetic field strength during the spin
manipulation pulse.Comment: 5 pages, 4 figure
Exploring Dark Matter with Milky Way substructure
The unambiguous detection of Galactic dark matter annihilation would unravel
one of the most outstanding puzzles in particle physics and cosmology. Recent
observations have motivated models in which the annihilation rate is boosted by
the Sommerfeld effect, a non-perturbative enhancement arising from a long range
attractive force. Here we apply the Sommerfeld correction to Via Lactea II, a
high resolution N-body simulation of a Milky-Way-size galaxy, to investigate
the phase-space structure of the Galactic halo. We show that the annihilation
luminosity from kinematically cold substructure can be enhanced by orders of
magnitude relative to previous calculations, leading to the prediction of
gamma-ray fluxes from up to hundreds of dark clumps that should be detectable
by the Fermi satellite.Comment: 23 pages, 9 figures (includes Supporting Online Material), accepted
for publication in Science, v2: added reference, fixed typo
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