Bibliographies thématiques / Dark Matter - Astroparticle Physics

Littérature scientifique sur le sujet « Dark Matter - Astroparticle Physics »

Auteur : Grafiati
Publié le 7 septembre 2023

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Articles de revues sur le sujet "Dark Matter - Astroparticle Physics"

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BETTINI, A. « ASTROPARTICLE PHYSICS ». International Journal of Modern Physics A 22, no 30 (10 décembre 2007) : 5550–60. http://dx.doi.org/10.1142/s0217751x07038815.

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Astroparticle is a very wide, expanding, sector of Physics; this report covers only a fraction of it complementing the plenary reports of Y. Takahashi and K. Inoue. I will focus, in particular, on the experimental evidence of new physics, beyond the Standard Model. Astroparticle and accelerator experiments will give complementary tools in the search of new particles, like those of the dark matter, and new fundamental fields, like the inflaton.
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Palanque-Delabrouille, Nathalie. « Overview of astroparticle physics and dark matter searches ». International Journal of Modern Physics A 22, no 31 (20 décembre 2007) : 5735–46. http://dx.doi.org/10.1142/s0217751x07038979.

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We present a general overview of recent results in the searches for dark matter and dark energy. We discuss the observation of the collision between two clusters of galaxies, and the impact this has on the relevance of dark matter. We then present the final results from microlensing experiments, which aimed at detecting dark baryonic objects in the halo of our galaxy, and the status of direct searches for WIMPs. We present the evidence for dark energy which initially comes from experiments dedicated to the study of distant type Ia supernovae. The measure of the baryon acoustic oscillation, an independent probe of the evolution of our universe that has recently brought interesting constraints, is finally described.
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Ko, Pyungwon. « Particle, Astroparticle Physics and Cosmology in Dark Matter Models with Dark Gauge Symmetries ». Journal of the Korean Physical Society 73, no 4 (août 2018) : 449–65. http://dx.doi.org/10.3938/jkps.73.449.

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Cho, A. « ASTROPARTICLE PHYSICS : Excess Particles From Space May Hint at Dark Matter ». Science 322, no 5905 (21 novembre 2008) : 1173. http://dx.doi.org/10.1126/science.322.5905.1173.

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Tinyakov, Peter, Maxim Pshirkov et Sergei Popov. « Astroparticle Physics with Compact Objects ». Universe 7, no 11 (25 octobre 2021) : 401. http://dx.doi.org/10.3390/universe7110401.

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Probing the existence of hypothetical particles beyond the Standard model often deals with extreme parameters: large energies, tiny cross-sections, large time scales, etc. Sometimes, laboratory experiments can test required regions of parameter space, but more often natural limitations lead to poorly restrictive upper limits. In such cases, astrophysical studies can help to expand the range of values significantly. Among astronomical sources, used in interests of fundamental physics, compact objects—neutron stars and white dwarfs—play a leading role. We review several aspects of astroparticle physics studies related to observations and properties of these celestial bodies. Dark matter particles can be collected inside compact objects resulting in additional heating or collapse. We summarize regimes and rates of particle capturing as well as possible astrophysical consequences. Then, we focus on a particular type of hypothetical particles—axions. Their existence can be uncovered due to observations of emission originated due to the Primakoff process in magnetospheres of neutron stars or white dwarfs. Alternatively, they can contribute to the cooling of these compact objects. We present results in these areas, including upper limits based on recent observations.
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Bignell, L. J., E. Barberio, M. B. Froehlich, G. J. Lane, O. Lennon, I. Mahmood, F. Nuti et al. « SABRE and the Stawell Underground Physics Laboratory Dark Matter Research at the Australian National University ». EPJ Web of Conferences 232 (2020) : 01002. http://dx.doi.org/10.1051/epjconf/202023201002.

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The direct detection of dark matter is a key problem in astroparticle physics that generally requires the use of deep-underground laboratories for a low-background environment where the rare signals from dark matter interactions can be observed. This work reports on the Stawell Underground Physics Laboratory – currently under construction and the first such laboratory in the Southern Hemisphere – and the associated research program. A particular focus will be given to ANU’s contribution to SABRE, a NaI:Tl dark matter, direct detection experiment that aims to confirm or refute the long-standing DAMA result. Preliminary measurements of the NaI:Tl quenching factor and characterisation of the SABRE liquid scintillator veto are reported.
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Moulin, Emmanuel. « Astroparticle Physics with H.E.S.S. : recents results and nearfuture prospects ». EPJ Web of Conferences 209 (2019) : 01054. http://dx.doi.org/10.1051/epjconf/201920901054.

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H.E.S.S. is an array of five Imaging Atmospheric Cherenkov Telescopes located in Namibia. It is designed for observations of astrophysical sources emitting very-high-energy (VHE) gamma rays in the energy range from a few ten GeVs to several ten TeVs. The H.E.S.S. instrument consists of four identical 12 m diameter telescopes and a 28 m diameter telescope placed at the center of the array. An ambitious Astroparticle Physics program is being carried out by the H.E.S.S. collaboration searching for New Physics in the VHE gamma-ray sky. The program includes the search for WIMP dark matter and axion-like particles, tests of Lorentz invariance, cosmic-ray electron measurements, and search for intergalactic magnetic fields. I will present the latest results on dark matter search from the observations of the Galactic Centre region, the search for Lorentz invariance violation with the 2014 flare observation of Markarian 501, and the first measurement of the cosmic-ray electron spectrum up to 20 TeV. The future of the H.E.S.S. Astroparticle Physics program will be discussed.
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Edwards, Thomas D. P., et Christoph Weniger. « A fresh approach to forecasting in astroparticle physics and dark matter searches ». Journal of Cosmology and Astroparticle Physics 2018, no 02 (12 février 2018) : 021. http://dx.doi.org/10.1088/1475-7516/2018/02/021.

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Jacob, Maurice. « The coming of age of cosmophysics ». Anais da Academia Brasileira de Ciências 75, no 2 (juin 2003) : 135–55. http://dx.doi.org/10.1590/s0001-37652003000200002.

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''Cosmophysics'' as reviewed is a multidisciplinary domain which brings together astroparticle physics, fundamental physics in space and topics related to the structure and evolution of the Universe. It represents a growing interface between high-energy particle physics and astro-physics. This paper presents a general overview of the subject, focusing on cosmology, cosmic rays, dark matter searches and the soon-expected observation of gravitational waves.
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Lapi, Andrea, Tommaso Ronconi, Lumen Boco, Francesco Shankar, Nicoletta Krachmalnicoff, Carlo Baccigalupi et Luigi Danese. « Astroparticle Constraints from Cosmic Reionization and Primordial Galaxy Formation ». Universe 8, no 9 (10 septembre 2022) : 476. http://dx.doi.org/10.3390/universe8090476.

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We derived astroparticle constraints in different dark matter scenarios that are alternatives to cold dark matter (CDM): thermal relic warm dark matter, WDM; fuzzy dark matter, ψDM; self-interacting dark matter, SIDM; sterile neutrino dark matter, νDM. Our framework is based on updated determinations of the high-redshift UV luminosity functions for primordial galaxies to redshift z∼10, on redshift-dependent halo mass functions in the above DM scenarios from numerical simulations, and on robust constraints on the reionization history of the Universe from recent astrophysical and cosmological datasets. First, we built an empirical model of cosmic reionization characterized by two parameters, namely the escape fraction fesc of ionizing photons from primordial galaxies, and the limiting UV magnitude MUVlim down to which the extrapolated UV luminosity functions steeply increased. Second, we performed standard abundance matching of the UV luminosity function and the halo mass function, obtaining a relationship between UV luminosity and the halo mass, whose shape depends on an astroparticle quantity X specific to each DM scenario (e.g., WDM particle mass); we exploited such a relationship to introduce (in the analysis) a constraint from primordial galaxy formation, in terms of the threshold halo mass above which primordial galaxies can efficiently form stars. Third, we performed Bayesian inference on the three parameters fesc, MUVlim, and X via a standard MCMC technique, and compared the outcomes of different DM scenarios on the reionization history. We also investigated the robustness of our findings against educated variations of still uncertain astrophysical quantities. Finally, we highlight the relevance of our astroparticle estimates in predicting the behavior of the high-redshift UV luminosity function at faint, yet unexplored magnitudes, which may be tested with the advent of the James Webb Space Telescope.
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Thèses sur le sujet "Dark Matter - Astroparticle Physics"

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Sivertsson, Sofia. « Dark matter in and around stars ». Licentiate thesis, Stockholm : Skolan för teknikvetenskap, Kungliga Tekniska högskolan, 2009. http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-11259.

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Burgess, Thomas. « A Search for Solar Neutralino Dark Matter with the AMANDA-II Neutrino Telescope ». Doctoral thesis, Stockholm : Physics Department, Stockholm University, 2008. http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-7378.

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Kahlhoefer, Felix Karl David. « Complementarity of searches for dark matter ». Thesis, University of Oxford, 2014. http://ora.ox.ac.uk/objects/uuid:ec5b1afe-b75c-44d9-9dad-e0d342e46fa1.

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The striking evidence for the existence of dark matter in the Universe implies that there is new physics to be discovered beyond the Standard Model. To identify the nature of this dark matter is a key task for modern astroparticle physics, and a large number of experiments pursuing a range of different search strategies have been developed to solve it. The topic of this thesis is the complementarity of these different experiments and the issue of how to combine the information from different searches independently of experimental and theoretical uncertainties. The first part focuses on the direct detection of dark matter scattering in nuclear recoil detectors, with a special emphasis on the impact of the assumed velocity distribution of Galactic dark matter particles. By converting experimental data to variables that make the astrophysical unknowns explicit, different experiments can be compared without implicit assumptions concerning the dark matter halo. We extend this framework to include annual modulation signals and apply it to recent experimental hints for dark matter, showing that the tension between these results and constraints from other experiments is independent of astrophysical uncertainties. We explore possible ways of ameliorating this tension by changing our assumptions on the properties of dark matter interactions. In this context, we propose a new approach for inferring the properties of the dark matter particle, which does not require any assumptions about the structure of the dark matter halo. A particularly interesting option is to study dark matter particles that couple differently to protons and neutrons (so-called isospin-violating dark matter). Such isospin-violation arises naturally in models where the vector mediator is the gauge boson of a new U(1) that mixes with the Standard Model gauge bosons. In the second part, we first discuss the case where both the Z' and the dark matter particle have a mass of a few GeV and then turn to the case where the Z' is significantly heavier. While the former case is most strongly constrained by precision measurements from LEP and B-factories, the latter scenario can be probed with great sensitivity at the LHC using monojet and monophoton searches, as well as searches for resonances in dijet, dilepton and diboson final states. Finally, we study models of dark matter where loop contributions are important for a comparison of LHC searches and direct detection experiments. This is the case for dark matter interactions with Yukawa-like couplings to quarks and for interactions that lead to spin-dependent or momentum suppressed scattering cross sections at tree level. We find that including the contribution from heavy-quark loops can significantly alter the conclusions obtained from a tree-level analysis.
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Buchholz, Annika [Verfasser]. « Various Aspects of Astroparticle Physics and the Implications for Dark Matter Searches / Annika Buchholz ». Bonn : Universitäts- und Landesbibliothek Bonn, 2020. http://d-nb.info/1218301287/34.

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Scott, Pat. « Searches for Particle Dark Matter Dark stars, dark galaxies, dark halos and global supersymmetric fits / ». Doctoral thesis, Stockholm : Department of Physics, Stockholm University, 2010. http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-38221.

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Diss. (sammanfattning) Stockholm : Stockholms universitet, 2010.
At the time of the doctoral defense, the following papers were unpublished and had a status as follows: Paper 5: Accepted. Paper 6: Submitted. Härtill 6 uppsatser.
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Lundström, Erik. « Phenomenology of Inert Scalar and Supersymmetric Dark Matter ». Doctoral thesis, Stockholms universitet, Fysikum, 2010. http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-39278.

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While the dark matter has so far only revealed itself through the gravitational influence it exerts on its surroundings, there are good reasons to believe it is made up by WIMPs – a hypothetical class of heavy elementary particles not encompassed by the Standard Model of particle physics. The Inert Doublet Model constitutes a simple extension of the Standard Model Higgs sector. The model provides a new set of scalar particles, denoted inert scalars because of their lack of direct coupling to matter, of which the lightest is a WIMP dark matter candidate. Another popular Standard Model extension is that of supersymmetry. In the most minimal scenario the particle content is roughly doubled, and the lightest of the new supersymmetric particles, which typically is a neutralino, is a WIMP dark matter candidate. In this thesis the phenomenology of inert scalar and supersymmetric dark matter is studied. Relic density calculations are performed, and experimental signatures in indirect detection experiments and accelerator searches are derived. The Inert Doublet Model shows promising prospects for indirect detection of dark matter annihilations into monochromatic photons. It is also constrained by the old LEP II accelerator data. Some phenomenological differences between the Minimal Supersymmetric Standard Model and a slight extension, the Beyond the Minimal Supersymmetric Standard Model, can be found. Also, supersymmetric dark matter models can be detected already within the early LHC accelerator data.
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Wikström, Gustav. « A search for solar dark matter with the IceCube neutrino telescope ». Doctoral thesis, Stockholms universitet, Fysikum, 2009. http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-27352.

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Dark matter particles in the form of supersymmetric Weakly Interacting Massive Particles (WIMPs) could accumulate in the centre of the Sun because of gravitational trapping. Pair-wise annihilations of WIMPs could create standard model particles out of which neutrinos could reach the Earth. Data from the IceCube 22-string neutrino telescope have been searched for signals from dark matter annihilations in the Sun. Highly sophisticated analysis methods have been developed to discern signal neutrinos from the severe background of atmospheric particle showers. No signal has been found in a dataset of 104 days livetime taken in 2007, and an upper limit has been placed on the muon flux in the South Pole ice induced by neutrinos from the Sun, reaching down to 330 km-2y-1. The flux limit has been converted into an upper limit on the neutralino scattering cross-section, which reaches down to 2.8*10-40 cm2 for spin-dependent interactions.
Four articles are appended to the thesis:I. G. Wikström for the IceCube collaboration, Proc. of the 30th ICRC,arXiv/0711.0353 [astro-ph] (2007) 135.II. A. Gross, C. Ha, C. Rott, M. Tluczykont, E. Resconi, T. DeYoung and G. Wikström for the IceCube Collaboration, Proc. of the 30th ICRC,arXiv/0711.0353 [astro-ph] (2007) 11.III. G. Wikström and J. Edsjö, JCAP 04 (2009) 009.IV. R. Abbasi et al. (IceCube collaboration), accepted for publication in Phys. Rev. Lett., arXiv/0902.2460v3 [astro-ph.CO] (2009).
IceCube
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Akrami, Yashar. « Supersymmetry vis-à-vis Observation : Dark Matter Constraints, Global Fits and Statistical Issues ». Doctoral thesis, Stockholms universitet, Fysikum, 2011. http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-57194.

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Weak-scale supersymmetry is one of the most favoured theories beyond the Standard Model of particle physics that elegantly solves various theoretical and observational problems in both particle physics and cosmology. In this thesis, I describe the theoretical foundations of supersymmetry, issues that it can address and concrete supersymmetric models that are widely used in phenomenological studies. I discuss how the predictions of supersymmetric models may be compared with observational data from both colliders and cosmology. I show why constraints on supersymmetric parameters by direct and indirect searches of particle dark matter are of particular interest in this respect. Gamma-ray observations of astrophysical sources, in particular dwarf spheroidal galaxies, by the Fermi satellite, and recording nuclear recoil events and energies by future ton-scale direct detection experiments are shown to provide powerful tools in searches for supersymmetric dark matter and estimating supersymmetric parameters. I discuss some major statistical issues in supersymmetric global fits to experimental data. In particular, I further demonstrate that existing advanced scanning techniques may fail in correctly mapping the statistical properties of the parameter spaces even for the simplest supersymmetric models. Complementary scanning methods based on Genetic Algorithms are proposed.
At the time of the doctoral defense, the following paper was unpublished and had a status as follows: Paper 4: Submitted.
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Ylinen, Tomi. « Search for Gamma-ray Lines from Dark Matter with the Fermi Large Area Telescope ». Doctoral thesis, KTH, Partikel- och astropartikelfysik, 2010. http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-12853.

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Dark matter (DM) constitutes one of the most intriguing but so far unresolved issues in physics. In many extensions of the Standard Model of particle physics, the existence of a stable Weakly Interacting Massive Particle (WIMP) is predicted. The WIMP is an excellent DM particle candidate. One of the most interesting scenarios is the creation of monochromatic gamma-rays from the annihilation or decay of these particles. This type of signal would represent a “smoking gun” for DM, since no other known astrophysical process should be able to produce it. In this thesis, the search for spectral lines with the Large Area Telescope (LAT) onboard the Fermi Gamma-ray Space Telescope (Fermi) is presented. The satellite was successfully launched from Cape Canaveral in Florida, USA, on 11 June, 2008. The energy resolution and performance of the detector are both key factors in the search and are investigated here using beam test data, taken at CERN in 2006 with a scaled-down version of the Fermi-LAT instrument. A variety of statistical methods, based on both hypothesis tests and confidence interval calculations, are then reviewed and tested in terms of their statistical power and coverage. A selection of the statistical methods are further developed into peak finding algorithms and applied to a simulated data set called obssim2, which corresponds to one year of observations with the Fermi-LAT instrument, and to almost one year of Fermi-LAT data in the energy range 20–300 GeV. The analysis on Fermi-LAT data yielded no detection of spectral lines, so limits are placed on the velocity-averaged cross-section, , and the decay lifetime, , and theoretical implications are discussed.
QC20100525
GLAST
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Sellerholm, Alexander. « Cosmological dark matter and the isotropic gamma-ray background measurements and upper limits / ». Doctoral thesis, Stockholm : Department of Physics, Stockholm University, 2010. http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-38900.

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Livres sur le sujet "Dark Matter - Astroparticle Physics"

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1942-, Klapdor-Kleingrothaus H. V., et Lewis Geraint F, dir. Dark matter in astroparticle and particle physics : Dark 2007, proceedings of the 6th International Heidelberg Conference, University of Sydney, Australia, 24-28 September 2007. Singapore : World Scientific, 2008.

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Lynden-Bell, D. Baryonic Dark Matter. Dordrecht : Springer Netherlands, 1990.

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Allen, Srednicki Mark, dir. Particle physics and cosmology : Dark matter. Amsterdam : North-Holland, 1990.

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Klapdor-Kleingrothaus, H. V., et R. D. Viollier, dir. Dark Matter in Astro- and Particle Physics. Berlin, Heidelberg : Springer Berlin Heidelberg, 2002. http://dx.doi.org/10.1007/978-3-642-55739-2.

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Klapdor-Kleingrothaus, H. V., dir. Dark Matter in Astro- and Particle Physics. Berlin, Heidelberg : Springer Berlin Heidelberg, 2001. http://dx.doi.org/10.1007/978-3-642-56643-1.

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Klapdor-Kleingrothaus, Hans Volker, et Richard Arnowitt, dir. Dark Matter in Astro- and Particle Physics. Berlin, Heidelberg : Springer Berlin Heidelberg, 2006. http://dx.doi.org/10.1007/b137487.

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Einstein and Hilbert : Dark matter. Hauppauge, N.Y : Nova Science Publishers, 2011.

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1975-, Bertone Gianfranco, dir. Particle dark matter : Observations, models and searches. New York : Cambridge University Press, 2009.

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Bertone, Gianfranco. Particle dark matter : Observations, models and searches. New York : Cambridge University Press, 2009.

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1965-, Kamionkowski Marc, Turner Michael S et United States. National Aeronautics and Space Administration., dir. Supersymmetric dark matter above the W mass. Batavia, IL : Fermi National Accelerator Laboratory, 1990.

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Chapitres de livres sur le sujet "Dark Matter - Astroparticle Physics"

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Grupen, Claus. « Dark Energy and Dark Matter ». Dans Astroparticle Physics, 401–34. Cham : Springer International Publishing, 2020. http://dx.doi.org/10.1007/978-3-030-27339-2_13.

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Mohanty, Subhendra. « Dark Matter ». Dans Astroparticle Physics and Cosmology, 9–48. Cham : Springer International Publishing, 2020. http://dx.doi.org/10.1007/978-3-030-56201-4_2.

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Sigl, Günter. « Dark Matter ». Dans Atlantis Studies in Astroparticle Physics and Cosmology, 711–53. Paris : Atlantis Press, 2016. http://dx.doi.org/10.2991/978-94-6239-243-4_14.

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Berezinsky, V. S. « Dark Matter and High Energy Neutrinos ». Dans Trends in Astroparticle-Physics, 243–64. Wiesbaden : Vieweg+Teubner Verlag, 1994. http://dx.doi.org/10.1007/978-3-663-01466-9_22.

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BISESI, ERICA, MOSÈ MARIOTTI et VILLI SCALZOTTO. « DARK MATTER DETECTION IN GAMMA ASTROPARTICLE EXPERIMENTS ». Dans Frontiers of Fundamental Physics, 315–20. Dordrecht : Springer Netherlands, 2006. http://dx.doi.org/10.1007/1-4020-4339-2_44.

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Bambi, Cosimo, et Alexandre D. Dolgov. « Dark Matter ». Dans UNITEXT for Physics, 175–89. Berlin, Heidelberg : Springer Berlin Heidelberg, 2015. http://dx.doi.org/10.1007/978-3-662-48078-6_9.

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Sidharth, B. G., et Abhishek Das. « Dark Matter Anomaly ». Dans Fundamental Physics and Physics Education Research, 77–83. Cham : Springer International Publishing, 2020. http://dx.doi.org/10.1007/978-3-030-52923-9_8.

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De Angelis, Alessandro, et Mário Pimenta. « The Standard Model of Cosmology and the Dark Universe ». Dans Introduction to Particle and Astroparticle Physics, 455–542. Cham : Springer International Publishing, 2018. http://dx.doi.org/10.1007/978-3-319-78181-5_8.

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De Angelis, Alessandro, et Mário João Martins Pimenta. « The Standard Model of Cosmology and the Dark Universe ». Dans Introduction to Particle and Astroparticle Physics, 421–504. Milano : Springer Milan, 2015. http://dx.doi.org/10.1007/978-88-470-2688-9_8.

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Turner, Michael S. « Dark Matter Candidates ». Dans Astronomy, Cosmology and Fundamental Physics, 279–86. Dordrecht : Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-009-0965-6_18.

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Actes de conférences sur le sujet "Dark Matter - Astroparticle Physics"

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Matsumoto, Shigeki. « Explosive dark matter annihilation ». Dans International Workshop on Astroparticle and High Energy Physics. Trieste, Italy : Sissa Medialab, 2003. http://dx.doi.org/10.22323/1.010.0044.

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Boehm, Celine. « A Light Dark Matter signature ? » Dans International Workshop on Astroparticle and High Energy Physics. Trieste, Italy : Sissa Medialab, 2003. http://dx.doi.org/10.22323/1.010.0065.

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Morselli, Aldo. « Search of dark matter with space experiments ». Dans International Workshop on Astroparticle and High Energy Physics. Trieste, Italy : Sissa Medialab, 2003. http://dx.doi.org/10.22323/1.010.0024.

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Fornengo, Nicolao. « Supersymmetric dark matter with gaugino non-universality ». Dans International Workshop on Astroparticle and High Energy Physics. Trieste, Italy : Sissa Medialab, 2003. http://dx.doi.org/10.22323/1.010.0056.

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Drobyshevski, Edward. « Detection and study of dark electric matter objects (daemons) ». Dans International Workshop on Astroparticle and High Energy Physics. Trieste, Italy : Sissa Medialab, 2003. http://dx.doi.org/10.22323/1.010.0077.

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MUNOZ, CARLOS. « Theoretical predictions for the direct detection of supersymmetric dark matter ». Dans International Workshop on Astroparticle and High Energy Physics. Trieste, Italy : Sissa Medialab, 2003. http://dx.doi.org/10.22323/1.010.0076.

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PINFOLD, JAMES L. « THE SYNERGY BETWEEN ASTROPARTICLE AND COLLIDER PHYSICS IN THE SEARCH FOR DARK MATTER ». Dans Proceedings of the 12th ICATPP Conference. WORLD SCIENTIFIC, 2011. http://dx.doi.org/10.1142/9789814329033_0030.

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Valle, J. W. F. « Neutrinos in astroparticle physics ». Dans THE DARK SIDE OF THE UNIVERSE : 2nd International Conference on The Dark Side of the Universe DSU 2006. AIP, 2006. http://dx.doi.org/10.1063/1.2409109.

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White, Simon. « Dark Matter ». Dans 26th Solvay Conference on Physics : “Astrophysics and Cosmology”. WORLD SCIENTIFIC, 2016. http://dx.doi.org/10.1142/9789814759182_0005.

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Dixon, Roger L. « Detecting dark matter ». Dans Instrumentation in elementary particle physics. AIP, 2000. http://dx.doi.org/10.1063/1.1361765.

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Rapports d'organisations sur le sujet "Dark Matter - Astroparticle Physics"

1

Witherell, Michael. Experimental High Energy Physics Research : Direct Detection of Dark Matter. Office of Scientific and Technical Information (OSTI), octobre 2014. http://dx.doi.org/10.2172/1158940.

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Kolb, Rocky, Harry Weerts, Natalia Toro, Richard Van de Water, Rouven Essig, Dan McKinsey, Kathryn Zurek et al. Basic Research Needs for Dark-Matter Small Projects New Initiatives : Report of the Department of Energy’s High Energy Physics Workshop on Dark Matter. Office of Scientific and Technical Information (OSTI), octobre 2018. http://dx.doi.org/10.2172/1659757.

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West, G. B. Dark matter and the solar neutrino problem : Can particle physics provide a single solution. Office of Scientific and Technical Information (OSTI), janvier 1989. http://dx.doi.org/10.2172/5556822.

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Noyes, H. P. Bit-string physics prediction of {eta}, the dark matter/baryon ratio and {Omega}{sub M}. Office of Scientific and Technical Information (OSTI), mars 2000. http://dx.doi.org/10.2172/753309.

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Argüelles, C. A., A. J. Aurisano, B. Batell, J. Berger, M. Bishai, T. Boschi, N. Byrnes et al. White Paper on New Opportunities at the Next-Generation Neutrino Experiments (Part 1 : BSM Neutrino Physics and Dark Matter). Office of Scientific and Technical Information (OSTI), juillet 2019. http://dx.doi.org/10.2172/1556972.

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Farbin, Amir. DoE Early Career Research Program : Final Report : Model-Independent Dark-Matter Searches at the ATLAS Experiment and Applications of Many-core Computing to High Energy Physics. Office of Scientific and Technical Information (OSTI), juillet 2015. http://dx.doi.org/10.2172/1193786.

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