3,200 research outputs found
On dark matter search after DAMA with Ge-73
The Weakly Interacting Massive Particle (WIMP) is one of the main candidates
for the relic dark matter (DM).In the effective low-energy minimal
supersymmetric standard model (effMSSM) the neutralino-nucleon spin and scalar
cross sections in the low-mass regime were calculated. The calculated cross
sections are compared with almost all experimental currently available
exclusion curves for spin-dependent WIMP-proton and WIMP-neutron cross
sections. It is demonstrated that in general about two-orders-of-magnitude
improvement of the current DM experiment sensitivities is needed to reach the
(effMSSM) SUSY predictions. At the current level of accuracy it looks
reasonable to safely neglect sub-dominant spin WIMP-nucleon contributions
analyzing the data from spin-non-zero targets. To avoid misleading
discrepancies between data and SUSY calculations it is, however, preferable to
use a mixed spin-scalar coupling approach.This approach is applied to estimate
future prospects of experiments with the odd-neutron high-spin isotope Ge-73.
It is noticed that the DAMA evidence favors the light Higgs sector in the
effMSSM, a high event rate in a Ge-73 detector and relatively high upgoing muon
fluxes from relic neutralino annihilations in the Earth and the Sun.Comment: 29 pages, 12 figures, 124 reference
One needs positive signatures for detection of Dark Matter
One believes there is huge amount of Dark Matter particles in our Galaxy
which manifest themselves only gravitationally. There is a big challenge to
prove their existence in a laboratory experiment. To this end it is not
sufficient to fight only for the best exclusion curve, one has to see an annual
recoil spectrum modulation --- the only available positive direct dark matter
detection signature. A necessity to measure the recoil spectra is stressed.Comment: 16 pages, 1 figure. arXiv admin note: substantial Appendix text
overlap with arXiv:0806.3917; missed acknowledge is added onl
Refined gluino and squark pole masses beyond leading order
The physical pole and running masses of squarks and gluinos have recently
been related at two-loop order in a mass-independent renormalization scheme. I
propose a general method for improvement of such formulas, and argue that
better accuracy results. The improved version gives an imaginary part of the
pole mass that agrees exactly with the direct calculation of the physical width
at next-to-leading order. I also find the leading three-loop contributions to
the gluino pole mass in the case that squarks are heavier, using effective
field theory and renormalization group methods. The efficacy of these
improvements for the gluino and squarks is illustrated with numerical examples.
Some necessary three-loop results for gauge coupling and fermion mass beta
functions and pole masses in theories with more than one type of fermion
representation, which are not directly accessible from the published
literature, are presented in an Appendix.Comment: 14 pages. v2: typos in equations (A.11), (A.17), and (A.18) fixe
Two-loop scalar self-energies and pole masses in a general renormalizable theory with massless gauge bosons
I present the two-loop self-energy functions for scalar bosons in a general
renormalizable theory, within the approximation that vector bosons are treated
as massless or equivalently that gauge symmetries are unbroken. This enables
the computation of the two-loop physical pole masses of scalar particles in
that approximation. The calculations are done simultaneously in the
mass-independent \bar{MS}, \bar{DR}, and \bar{DR}' renormalization schemes, and
with arbitrary covariant gauge fixing. As an example, I present the two-loop
SUSYQCD corrections to squark masses, which can increase the known one-loop
results by of order one percent. More generally, it is now straightforward to
implement all two-loop sfermion pole mass computations in supersymmetry using
the results given here, neglecting only the electroweak vector boson masses
compared to the superpartner masses in the two-loop parts.Comment: 16 pages, 4 figures. v2: typo in eq. (5.30) fixe
Direct Search for Dark Matter - Striking the Balance - and the Future
Weakly Interacting Massive Particles (WIMPs) are among the main candidates
for the relic dark matter (DM). The idea of the direct DM detection relies on
elastic spin-dependent (SD) and spin-independent (SI) interaction of WIMPs with
target nuclei. In this review paper the relevant formulae for WIMP event rate
calculations are collected. For estimations of the WIMP-proton and WIMP-neutron
SD and SI cross sections the effective low-energy minimal supersymmetric
standard model is used. The traditional one-coupling-dominance approach for
evaluation of the exclusion curves is described. Further, the mixed spin-scalar
coupling approach is discussed. It is demonstrated, taking the high-spin Ge-73
dark matter experiment HDMS as an example, how one can drastically improve the
sensitivity of the exclusion curves within the mixed spin-scalar coupling
approach, as well as due to a new procedure of background subtraction from the
measured spectrum. A general discussion on the information obtained from
exclusion curves is given. The necessity of clear WIMP direct detection
signatures for a solution of the dark matter problem, is pointed out.Comment: LaTeX, 49 pages, 14 figures, 185 reference
Two-loop SUSY QCD corrections to the chargino masses in the MSSM
We have calculated the two-loop strong interaction corrections to the
chargino pole masses in the DRbar'-scheme in the Minimal Supersymmetric
Standard Model (MSSM) with complex parameters. We have performed a detailed
numerical analysis for a particular point in the parameter space and found
corrections of a few tenths of a percent. We provide a computer program which
calculates chargino and neutralino masses with complex parameters including the
one-loop corrections and all two-loop SQCD effects.Comment: 12 pages, 11 figures, references modified, clarifications adde
About direct Dark Matter detection in Next-to-Minimal Supersymmetric Standard Model
Direct dark matter detection is considered in the Next-to-Minimal
Supersymmetric Standard Model (NMSSM). The effective neutralino-quark
Lagrangian is obtained and event rates are calculated for the Ge-73 isotope.
Accelerator and cosmological constraints on the NMSSM parameter space are
included. By means of scanning the parameter space at the Fermi scale we show
that the lightest neutralino could be detected in dark matter experiments with
sizable event rate.Comment: latex, 12 pages, 2 ps-figures; extra LEP constraint is included,
extra figure is added, recorrected version, resubmitted to Phys.Rev.
Squark-, Slepton- and Neutralino-Chargino coannihilation effects in the low-energy effective MSSM
Within the low-energy effective Minimal Supersymmetric extension of the
Standard Model (effMSSM) we calculate the neutralino relic density taking into
account slepton-neutralino, squark-neutralino and neutralino/chargino-
neutralino coannihilation channels. By including squark (stop and sbottom)
coannihilation channels we extend our comparative study to all allowed
coannihilations and obtain the general result that all of them give sizable
contributions to the reduction of the neutralino relic density. Due to these
coannihilation processes some models (mostly with large neutralino masses)
enter into the cosmologically interesting region for relic density, but other
models leave this region. Nevertheless, in general, the predictions for direct
and indirect dark matter detection rates are not strongly affected by these
coannihilation channels in the effMSSM.Comment: 14 pages, 10 figures, corrected and to be published in Phys. Rev.
Slepton and Neutralino/Chargino Coannihilations in MSSM
Within the low-energy effective Minimal Supersymmetric extension of Standard
Model (effMSSM) we calculated the neutralino relic density taking into account
slepton-neutralino and neutralino-chargino/neutralino coannihilation channels.
We performed comparative study of these channels and obtained that both of them
give sizable contributions to the reduction of the relic density. Due to these
coannihilation processes some models (mostly with large neutralino masses)
enter into the cosmologically interesting region for relic density, but other
models leave this region. Nevertheless, in general, the predictions for direct
and indirect dark matter detection rates are not strongly affected by these
coannihilation channels in the effMSSM.Comment: 12 pages, 9 figures, revte
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