3,559 research outputs found
Electroweak Bremsstrahlung in Dark Matter Annihilation
A conservative upper bound on the total dark matter (DM) annihilation rate
can be obtained by constraining the appearance rate of the annihilation
products which are hardest to detect. The production of neutrinos, via the
process , has thus been used to set a strong
general bound on the dark matter annihilation rate. However, Standard Model
radiative corrections to this process will inevitably produce photons which may
be easier to detect. We present an explicit calculation of the branching ratios
for the electroweak bremsstrahlung processes and
. These modes inevitably lead to electromagnetic
showers and further constraints on the DM annihilation cross-section. In
addition to annihilation, our calculations are also applicable to the case of
dark matter decay.Comment: 7 pages, 4 figures. New appendix with an extensive discussion of
Majorana fermions and helicity suppression
The Scientific Reach of Multi-Ton Scale Dark Matter Direct Detection Experiments
The next generation of large scale WIMP direct detection experiments have the
potential to go beyond the discovery phase and reveal detailed information
about both the particle physics and astrophysics of dark matter. We report here
on early results arising from the development of a detailed numerical code
modeling the proposed DARWIN detector, involving both liquid argon and xenon
targets. We incorporate realistic detector physics, particle physics and
astrophysical uncertainties and demonstrate to what extent two targets with
similar sensitivities can remove various degeneracies and allow a determination
of dark matter cross sections and masses while also probing rough aspects of
the dark matter phase space distribution. We find that, even assuming dominance
of spin-independent scattering, multi-ton scale experiments still have
degeneracies that depend sensitively on the dark matter mass, and on the
possibility of isospin violation and inelasticity in interactions. We find that
these experiments are best able to discriminate dark matter properties for dark
matter masses less than around 200 GeV. In addition, and somewhat surprisingly,
the use of two targets gives only a small improvement (aside from the advantage
of different systematics associated with any claimed signal) in the ability to
pin down dark matter parameters when compared with one target of larger
exposure.Comment: 23 pages; updated to match PRD versio
Searching for Dark Matter at the LHC with a Mono-Z
We investigate a mono-Z process as a potential dark matter search strategy at
the LHC. In this channel a single Z boson recoils against missing transverse
momentum, attributed to dark matter particles, , which escape the
detector. This search strategy is related, and complementary to, monojet and
monophoton searches. For illustrative purposes we consider the process
in a toy dark matter model, where the Z boson is
emitted from either the initial state quarks, or from the internal propagator.
Among the signatures of this process will be a pair of muons with high pT that
reconstruct to the invariant mass of the Z, and large amounts of missing
transverse energy. Being a purely electroweak signal, QCD and other Standard
Model backgrounds are relatively easily removed with modest selection cuts. We
compare the signal to Standard Model backgrounds and demonstrate that, even for
conservative cuts, there exist regions of parameter space where the signal may
be clearly visible above background in future LHC data, allowing either new
discovery potential or the possibility of supplementing information about the
dark sector beyond that available from other observable channels.Comment: 11 pages, 13 figure
Dark Matter Annihilation Signatures from Electroweak Bremsstrahlung
We examine observational signatures of dark matter annihilation in the Milky
Way arising from electroweak bremsstrahlung contributions to the annihilation
cross section. It has been known for some time that photon bremsstrahlung may
significantly boost DM annihilation yields. Recently, we have shown that
electroweak bremsstrahlung of W and Z gauge bosons can be the dominant
annihilation channel in some popular models with helicity-suppressed 2 --> 2
annihilation. W/Z-bremsstrahlung is particularly interesting because the gauge
bosons produced via annihilation subsequently decay to produce large correlated
fluxes of electrons, positrons, neutrinos, hadrons (including antiprotons) and
gamma rays, which are all of importance in indirect dark matter searches. Here
we calculate the spectra of stable annihilation products produced via
gamma/W/Z-bremsstrahlung. After modifying the fluxes to account for the
propagation through the Galaxy, we set upper bounds on the annihilation cross
section via a comparison with observational data. We show that stringent cosmic
ray antiproton limits preclude a sizable dark matter contribution to observed
cosmic ray positron fluxes in the class of models for which the bremsstrahlung
processes dominate.Comment: 11 pages, 6 figures. Updated to match PRD versio
Robust Constraints on Dark Matter Annihilation into Gamma Rays and Charged Particles
Using gamma-ray data from observations of the Milky Way, Andromeda (M31), and
the cosmic background, we calculate conservative upper limits on the dark
matter self-annihilation cross section to a number of final states, over a wide
range of dark matter masses. We first constrain annihilation to a pair of
monoenergetic gamma rays, and show that in general our results are unchanged
for a broader annihilation spectrum, if at least a few gamma rays are produced
with energies within a factor of a few from the dark matter mass. We then place
constraints on the self-annihilation cross section to an electron-positron
pair, using gamma rays produced via internal bremsstrahlung radiative
corrections. We also place constraints on annihilation into the other charged
leptons. We make conservative assumptions about the astrophysical inputs, and
demonstrate how our derived bounds would be strengthened if stronger
assumptions about these inputs are adopted.Comment: 7 pages, 5 figures. Talk given at DSU 09, Melbourne, Australia, June
200
An Approach to Catheter Ablation of Cavotricuspid Isthmus Dependent Atrial Flutter
Much of our understanding of the mechanisms of macro re-entrant atrial tachycardia comes from study of cavotricuspid isthmus (CTI) dependent atrial flutter. In the majority of cases, the diagnosis can be made from simple analysis of the surface ECG. Endocardial mapping during tachycardia allows confirmation of the macro re-entrant circuit within the right atrium while, at the same time, permitting curative catheter ablation targeting the critical isthmus of tissue located between the tricuspid annulus and the inferior vena cava. The procedure is short, safe and by demonstration of an electrophysiological endpoint - bidirectional conduction block across the CTI - is associated with an excellent outcome following ablation. It is now fair to say that catheter ablation should be considered as a first line therapy for patients with documented CTI-dependent atrial flutter
W/Z Bremsstrahlung as the Dominant Annihilation Channel for Dark Matter, Revisited
We revisit the calculation of electroweak bremsstrahlung contributions to
dark matter annihilation. Dark matter annihilation to leptons is necessarily
accompanied by electroweak radiative corrections, in which a or boson
is also radiated. Significantly, while many dark matter models feature a
helicity suppressed annihilation rate to fermions, bremsstrahlung process can
remove this helicity suppression such that the branching ratios Br(), Br(), and Br() dominate over
Br() and Br(). We find this is most significant in
the limit where the dark matter mass is nearly degenerate with the mass of the
boson which mediates the annihilation process. Electroweak bremsstrahlung has
important phenomenological consequences both for the magnitude of the total
dark matter annihilation cross section and for the character of the
astrophysical signals for indirect detection. Given that the and gauge
bosons decay dominantly via hadronic channels, it is impossible to produce
final state leptons without accompanying protons, antiprotons, and gamma rays.Comment: 8 pages, 6 figures; replaced to match published versio
W/Z Bremsstrahlung as the Dominant Annihilation Channel for Dark Matter
Dark matter annihilation to leptons, , is
necessarily accompanied by electroweak radiative corrections, in which a W or Z
boson is radiated from a final state particle. Given that the W and Z gauge
bosons decay dominantly via hadronic channels, it is thus impossible to produce
final state leptons without accompanying protons, antiprotons, and gamma rays.
Significantly, while many dark matter models feature a helicity suppressed
annihilation rate to fermions, radiating a massive gauge boson from a final
state fermion removes this helicity suppression, such that the branching ratios
Br(l \nu W), Br(l^+l^- Z), and Br(\nu\nubar Z) dominate over Br(l\bar{l}).
W/Z-bremsstrahlung thus allows indirect detection of many WIMP models that
would otherwise be helicity-suppressed, or v^2 suppressed. Antiprotons and even
anti-deuterons become consequential final state particles. This is an important
result for future DM searches. We discuss the implications of
W/Z-bremsstrahlung for "leptonic" DM models which aim to fit recent cosmic ray
positron and antiproton data.Comment: 19 pages, 5 figures. Updated to include Erratum, and changes made to
PRD versio
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