| 1. |
- Baltz, Edward A., et al.
(författare)
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Pre-launch estimates for GLAST sensitivity to Dark Matter annihilation signals
- 2008
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Ingår i: Journal of Cosmology and Astroparticle Physics. - : IOP Publishing. - 1475-7516. ; 0807:013
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Tidskriftsartikel (refereegranskat)abstract
- We investigate the sensitivity of the Gamma-ray Large Area Space Telescope (GLAST) for indirectly detecting weakly interacting massive particles (WIMPs) through the γ-ray signal that their pair annihilation produces. WIMPs are among the favorite candidates for explaining the compelling evidence that about 80% of the mass in the Universe is non-baryonic dark matter (DM). They are serendipitously motivated by various extensions of the standard model of particle physics such as supersymmetry and universal extra dimensions (UED). With its unprecedented sensitivity and its very large energy range (20 MeV to more than 300 GeV) the main instrument on board the GLAST satellite, the Large Area Telescope (LAT), will open a new window of discovery. As our estimates show, the LAT will be able to detect an indirect DM signature for a large class of WIMP models given a cuspy profile for the DM distribution. Using the current state of the art Monte Carlo and event reconstruction software developed within the LAT collaboration, we present preliminary sensitivity studies for several possible sources inside and outside the Galaxy. We also discuss the potential of the LAT to detect UED via the electron/positron channel. Diffuse background modeling and other background issues that will be important in setting limits or seeing a signal are presented
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| 2. |
- Berg, Marcus, et al.
(författare)
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Neutralino Dark Matter in BMSSM Effective Theory
- 2009
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Ingår i: Journal of Cosmology and Astroparticle Physics. - : IOP Publishing. - 1475-7516. ; :08
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Tidskriftsartikel (refereegranskat)abstract
- We study thermal neutralino dark matter in an effective field theory extension of the MSSM, called ``Beyond the MSSM'' (BMSSM) in Dine, Seiberg and Thomas (2007). In this class of effective field theories, the field content of the MSSM is unchanged, but the little hierarchy problem is alleviated by allowing small corrections to the Higgs/higgsino part of the Lagrangian. We perform parameter scans and compute the dark matter relic density. The light higgsino LSP scenario is modified the most; we find new regions of parameter space compared to the standard MSSM. This involves interesting interplay between the WMAP dark matter bounds and the LEP chargino bound. We also find some changes for gaugino LSPs, partly due to annihilation through a Higgs resonance, and partly due to coannihilation with light top squarks in models that are ruled in by the new effective terms.
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| 3. |
- Bergström, Lars, 1952-, et al.
(författare)
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Gamma-ray and Radio Constraints of High Positron Rate Dark Matter Models Annihilating into New Light Particles
- 2009
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Ingår i: Physical Review Letters. - 0031-9007 .- 1079-7114. ; 79:8, s. 081303-
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Tidskriftsartikel (refereegranskat)abstract
- The possibility of explaining the positron and electron excess recently found by the PAMELA and ATIC collaborations in terms of dark matter (DM) annihilation has attracted considerable attention. Models surviving bounds from, e.g, antiproton production generally fall into two classes, where either DM annihilates directly with a large branching fraction into light leptons, or, as in the recent models of Arkani-Hamed et al., and of Nomura and Thaler, the annihilation gives low-mass (pseudo)scalars or vectors $\phi$ which then decay into $\mu^+\mu^-$ or $e^+e^-$. While the constraints on the first kind of models have recently been treated by several authors, we study here specifically models of the second type which rely on an efficient Sommerfeld enhancement in order to obtain the necessary boost in the annihilation cross section. We compute the photon flux generated by QED radiative corrections to the decay of $\phi$ and show that this indeed gives a rather spectacular broad peak in $E^2d\sigma/dE$, that for these extreme values of the cross section violate gamma-ray observations of the Galactic center for DM density profiles steeper than that of Navarro, Frenk and White. The most stringent constraint comes from the comparison of the predicted synchrotron radiation in the central part of the Galaxy with radio observations of Sgr A*. For the most commonly adopted DM profiles, the models that provide a good fit to the PAMELA and ATIC data are ruled out, unless there are physical processes that boost the local anti-matter fluxes more than one order of magnitude, while not affecting the gamma-ray or radio fluxes.
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| 4. |
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| 5. |
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| 6. |
- Blennow, Mattias, et al.
(författare)
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Neutrinos from WIMP annihilations in the Sun including neutrino oscillations
- 2006
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Ingår i: Physica Scripta. - : IOP Publishing. - 0031-8949 .- 1402-4896. ; T127, s. 19-21
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Tidskriftsartikel (refereegranskat)abstract
- The prospects for detecting neutrinos from the Sun arising from dark matter annihilations in the core of the Sun are reviewed. Emphasis is placed on new work investigating the effects of neutrino oscillations on the expected neutrino fluxes.
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| 7. |
- Blennow, Mattias, et al.
(författare)
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WIMP neutrinos from the Sun and the Earth
- 2008
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Konferensbidrag (refereegranskat)abstract
- We discuss the propagation treatment of the indirect dark matter detection using WIMP annihilations in the Sun and the Earth. In particular, we focus on treating neutrino interactions and oscillations in a consistent framework, including tau neutrino regeneration and a full three-flavor neutrino oscillation framework. We also discuss the equivalence of using a Monte Carlo approach - suited for inclusion in neutrino telescope Monte Carlos - and the density matrix formalism.
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| 8. |
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| 9. |
- Gunnarsson, Christofer, 1976-
(författare)
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Supernovae under the gravitational lens
- 2005
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Doktorsavhandling (övrigt vetenskapligt/konstnärligt)abstract
- With general relativity as its foundation, the Standard Model of Cosmology has been developed, a model in which all matter is homogeneously and isotropically distributed throughout the Universe. We know for sure that this is not true since inhomogeneous structures such as galaxies, planets and synthesizers, are known to exist on small cosmological scales. However, on large scales the approximation of homogeneity is very good. Despite this, inhomogeneities such as galaxies or clusters of galaxies, will affect the propagation of light in the Universe by bending the paths of light-rays according to the laws of general relativity. The phenomenon is known as gravitational lensing. The bending of light-rays is similar to what happens in an optical lens, where an image of an object may be distorted or (de-)magnified depending on the shape of the lens.Using the magnifying power of a gravitational lens it is possible to see further out in the Universe, it is used as a natural gravitational telescope. Under the right circumstances this can be something very useful. By studying light from supernovae, exploding stars, it is to some extent possible to gather information on the constituents of our universe. If for some reason this light is affected on its way to us, e.g. by gravitational lensing, we are mislead into drawing erroneous conclusions unless the lensing effects are under control and corrected for. Trying to control this and other systematic uncertainties is a big challenge in supernova cosmology and is also becoming more and more important as statistical errors are being beaten down to very low levels.
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| 10. |
- Gustafsson, Michael, et al.
(författare)
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Significant Gamma Lines from Inert Higgs Dark Matter
- 2007
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Ingår i: Physical Review Letters. - : American Physical Society. ; 99:041301
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Tidskriftsartikel (refereegranskat)abstract
- One way to unambiguously confirm the existence of particle dark matter and determine its mass would be to detect its annihilation into monochromatic gamma-rays in upcoming telescopes. One of the most minimal models for dark matter is the inert doublet model, obtained by adding another Higgs doublet with no direct coupling to fermions. For a mass between 40 and 80 GeV, the lightest of the new inert Higgs particles can give the correct cosmic abundance of cold dark matter in agreement with current observations. We show that for this scalar dark matter candidate, the annihilation signal of monochromatic γγ and Zγ final states would be exceptionally strong. The energy range and rates for these gamma-ray line signals make them ideal to search for with the soon upcoming GLAST satellite.
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