Articles de revues : « Indirect Searches »

1

Barish, Barry C. « Indirect searches for dark matter ». Nuclear Physics B - Proceedings Supplements 77, n^o 1-3 (mai 1999) : 398–401. http://dx.doi.org/10.1016/s0920-5632(99)00449-1.

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CIRELLI, MARCO. « Indirect searches for dark matter ». Pramana 79, n^o 5 (27 octobre 2012) : 1021–43. http://dx.doi.org/10.1007/s12043-012-0419-x.

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Donato, Fiorenza. « Indirect searches for dark matter ». Physics of the Dark Universe 4 (septembre 2014) : 41–43. http://dx.doi.org/10.1016/j.dark.2014.06.001.

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Aguilar Sánchez, Juan Antonio. « Indirect Searches for Dark Matter with IceCube ». EPJ Web of Conferences 207 (2019) : 04006. http://dx.doi.org/10.1051/epjconf/201920704006.

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The nature of dark matter remains one of the unsolved questions in modern cosmology and to understand its properties different experimental avenues are being explored. Indirect searches make use of the annihilation or decay products of dark matter as tracers to prove its existence. Unlike direct detections methods, indirect searches do not require specialized detectors as existing astro-particle experiments and facilities can be used to search for signatures of dark matter. Among the decay and annihilation products, neutrinos offer a unique way to search for dark matter since their low cross-section makes them capable of escaping from environments in which gamma rays will be absorbed, like the Sun or the Earth. The IceCube neutrino telescope is not only an excellent astro-particle detector, it also has lively program on dark matter searches with very competitive and complementary results to direct detection limits. These proceedings review the latests results of IceCube regarding the indirect search of dark matter with neutrinos.

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BIGI, I. I. « Indirect Searches for Very Heavy Quarks ». Annals of the New York Academy of Sciences 518, n^o 1 The Fourth Fa (décembre 1987) : 75–81. http://dx.doi.org/10.1111/j.1749-6632.1987.tb48808.x.

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IBARRA, ALEJANDRO, DAVID TRAN et CHRISTOPH WENIGER. « INDIRECT SEARCHES FOR DECAYING DARK MATTER ». International Journal of Modern Physics A 28, n^o 27 (30 octobre 2013) : 1330040. http://dx.doi.org/10.1142/s0217751x13300408.

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Numerous observations point towards the existence of an unknown elementary particle with no electromagnetic interactions, a large population of which was presumably produced in the early stages of the history of the Universe. This so-called dark matter has survived until the present day, accounting for the 26% of the present energy budget of the Universe. It remains an open question whether the particles comprising the dark matter are absolutely stable or whether they have a finite but very long lifetime, which is a possibility since there is no known general principle guaranteeing perfect stability. In this paper, we review the observational limits on the lifetime of dark matter particles with mass in the GeV–TeV range using observations of the cosmic fluxes of antimatter, gamma-rays and neutrinos. We also examine some theoretically motivated scenarios that provide decaying dark matter candidates.

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Grefe, Michael. « Indirect searches for gravitino dark matter ». Journal of Physics : Conference Series 375, n^o 1 (30 juillet 2012) : 012035. http://dx.doi.org/10.1088/1742-6596/375/1/012035.

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Medici, Morten. « Indirect Dark Matter Searches with IceCube ». Journal of Physics : Conference Series 1342 (janvier 2020) : 012074. http://dx.doi.org/10.1088/1742-6596/1342/1/012074.

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Muñoz, Carlos. « Indirect dark matter searches and models ». Nuclear Instruments and Methods in Physics Research Section A : Accelerators, Spectrometers, Detectors and Associated Equipment 692 (novembre 2012) : 13–19. http://dx.doi.org/10.1016/j.nima.2012.01.053.

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Gorbunov, Dmitry, et Inar Timiryasov. « Testing ν MSM with indirect searches ». Physics Letters B 745 (mai 2015) : 29–34. http://dx.doi.org/10.1016/j.physletb.2015.02.060.

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Boezio, M., M. Pearce, P. Picozza, R. Sparvoli, P. Spillantini, O. Adriani, G. C. Barbarino et al. « PAMELA and indirect dark matter searches ». New Journal of Physics 11, n^o 10 (16 octobre 2009) : 105023. http://dx.doi.org/10.1088/1367-2630/11/10/105023.

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Serpico, Pasquale Dario. « (Indirect) dark matter searches : Status and challenges ». International Journal of Modern Physics E 30, n^o 07 (juillet 2021) : 2130002. http://dx.doi.org/10.1142/s0218301321300022.

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I summarize the rationale of dark matter searches as well as their main challenges, with a focus on indirect techniques. After briefly reviewing the status of current searches and without ambition of completeness, I present some personal perspectives on the directions of development in the field.

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Budnik, R. « Dark Matter : Evidence, Direct and Indirect Searches ». Acta Physica Polonica B 47, n^o 1 (2016) : 217. http://dx.doi.org/10.5506/aphyspolb.47.217.

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Cirelli, Marco. « Dark matter indirect searches : charged cosmic rays ». Journal of Physics : Conference Series 718 (mai 2016) : 022005. http://dx.doi.org/10.1088/1742-6596/718/2/022005.

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Weniger, Christoph, Torsten Bringmann, Francesca Calore et Gilles Vertongen. « Spectral cutoffs in indirect dark matter searches ». Journal of Physics : Conference Series 375, n^o 1 (30 juillet 2012) : 012034. http://dx.doi.org/10.1088/1742-6596/375/1/012034.

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Scholberg, K. « Indirect dark matter searches with AMS-02 ». Nuclear Physics B - Proceedings Supplements 138 (janvier 2005) : 35–37. http://dx.doi.org/10.1016/j.nuclphysbps.2004.11.007.

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Rott, C., et the IceCube Collaboration. « Indirect searches for dark matter with IceCube ». Journal of Physics : Conference Series 120, n^o 2 (1 juillet 2008) : 022009. http://dx.doi.org/10.1088/1742-6596/120/2/022009.

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Pérez de los Heros, Carlos. « Status, Challenges and Directions in Indirect Dark Matter Searches ». Symmetry 12, n^o 10 (8 octobre 2020) : 1648. http://dx.doi.org/10.3390/sym12101648.

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Indirect searches for dark matter are based on detecting an anomalous flux of photons, neutrinos or cosmic-rays produced in annihilations or decays of dark matter candidates gravitationally accumulated in heavy cosmological objects, like galaxies, the Sun or the Earth. Additionally, evidence for dark matter that can also be understood as indirect can be obtained from early universe probes, like fluctuations of the cosmic microwave background temperature, the primordial abundance of light elements or the Hydrogen 21-cm line. The techniques needed to detect these different signatures require very different types of detectors: Air shower arrays, gamma- and X-ray telescopes, neutrino telescopes, radio telescopes or particle detectors in balloons or satellites. While many of these detectors were not originally intended to search for dark matter, they have proven to be unique complementary tools for direct search efforts. In this review we summarize the current status of indirect searches for dark matter, mentioning also the challenges and limitations that these techniques encounter.

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Cirelli, Marco. « Dark Matter Indirect searches : phenomenological and theoretical aspects ». Journal of Physics : Conference Series 447 (24 juillet 2013) : 012006. http://dx.doi.org/10.1088/1742-6596/447/1/012006.

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Rizzo, Thomas G. « Indirect searches forZ′-like resonances at the LHC ». Journal of High Energy Physics 2009, n^o 08 (21 août 2009) : 082. http://dx.doi.org/10.1088/1126-6708/2009/08/082.

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Brun, P. « Indirect searches for dark matter with AMS-02 ». European Physical Journal C 56, n^o 1 (27 juin 2008) : 27–31. http://dx.doi.org/10.1140/epjc/s10052-008-0659-6.

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Ando, Shin’ichiro. « Dark matter indirect searches : Multi-wavelength and anisotropies ». Journal of Physics : Conference Series 718 (mai 2016) : 022002. http://dx.doi.org/10.1088/1742-6596/718/2/022002.

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Choubey, S., A. Ghosh et D. Tiwari. « Indirect Searches for Dark Matter Signatures at INO ». Journal of Physics : Conference Series 1342 (janvier 2020) : 012101. http://dx.doi.org/10.1088/1742-6596/1342/1/012101.

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Morselli, Aldo. « Indirect searches in the PAMELA and Fermi era ». Nuclear Physics B - Proceedings Supplements 194 (octobre 2009) : 105–10. http://dx.doi.org/10.1016/j.nuclphysbps.2009.07.009.

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BOTTINO, A., V. DE ALFARO, N. FORNENGO, A. MORALES, J. PUIMEDÓN et S. SCOPEL. « DIRECT VERSUS INDIRECT SEARCHES FOR NEUTRALINO DARK MATTER ». Modern Physics Letters A 07, n^o 09 (21 mars 1992) : 733–47. http://dx.doi.org/10.1142/s0217732392000707.

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Direct search for neutralino dark matter is analyzed in the framework of the minimal supersymmetric extension of the standard model, using a realistic evaluation of the neutralino relic abundance which also includes radiative corrections to the Higgs masses. Relevance of the present (Ge detectors) experimental data to set constraints on the parameters of the model is discussed and expectations for future experiments which involve neutralino-nucleus coherent processes are investigated. These results are compared to those obtained in a previous paper from indirect search data. In the present analysis particular attention is paid to the theoretical uncertainties due to the different estimates of the Higgs-nucleon coupling strength.

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Siegal-Gaskins, Jennifer M. « Separating astrophysical sources from indirect dark matter signals ». Proceedings of the National Academy of Sciences 112, n^o 40 (10 octobre 2014) : 12272–77. http://dx.doi.org/10.1073/pnas.1315181111.

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Indirect searches for products of dark matter annihilation and decay face the challenge of identifying an uncertain and subdominant signal in the presence of uncertain backgrounds. Two valuable approaches to this problem are (i) using analysis methods which take advantage of different features in the energy spectrum and angular distribution of the signal and backgrounds and (ii) more accurately characterizing backgrounds, which allows for more robust identification of possible signals. These two approaches are complementary and can be significantly strengthened when used together. I review the status of indirect searches with gamma rays using two promising targets, the Inner Galaxy and the isotropic gamma-ray background. For both targets, uncertainties in the properties of backgrounds are a major limitation to the sensitivity of indirect searches. I then highlight approaches which can enhance the sensitivity of indirect searches using these targets.

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27

Zornoza, Juan de Dios. « Review on Indirect Dark Matter Searches with Neutrino Telescopes ». Universe 7, n^o 11 (30 octobre 2021) : 415. http://dx.doi.org/10.3390/universe7110415.

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The search for dark matter is one of the hottest topics in Physics today. The fact that about 80% of the matter of the Universe is of unknown nature has triggered an intense experimental activity to detect this kind of matter and a no less intense effort on the theory side to explain it. Given the fact that we do not know the properties of dark matter well, searches from different fronts are mandatory. Neutrino telescopes are part of this experimental quest and offer specific advantages. Among the targets to look for dark matter, the Sun and the Galactic Center are the most promising ones. Considering models of dark matter densities in the Sun, neutrino telescopes have put the best limits on spin-dependent cross section of proton-WIMP scattering. Moreover, they are competitive in the constraints on the thermally averaged annihilation cross-section for high WIMP masses when looking at the Galactic Centre. Other results are also reviewed.

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Garcia-Cely, Camilo, et Julian Heeck. « Indirect searches of dark matter via polynomial spectral features ». Journal of Cosmology and Astroparticle Physics 2016, n^o 08 (11 août 2016) : 023. http://dx.doi.org/10.1088/1475-7516/2016/08/023.

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Bartels, Richard, Daniele Gaggero et Christoph Weniger. « Prospects for indirect dark matter searches with MeV photons ». Journal of Cosmology and Astroparticle Physics 2017, n^o 05 (2 mai 2017) : 001. http://dx.doi.org/10.1088/1475-7516/2017/05/001.

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Choubey, Sandhya, Anushree Ghosh et Deepak Tiwari. « Prospects of indirect searches for dark matter at INO ». Journal of Cosmology and Astroparticle Physics 2018, n^o 05 (2 mai 2018) : 006. http://dx.doi.org/10.1088/1475-7516/2018/05/006.

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Mijakowski, Piotr. « Indirect searches for dark matter particles at Super-Kamiokande ». Journal of Physics : Conference Series 718 (mai 2016) : 042040. http://dx.doi.org/10.1088/1742-6596/718/4/042040.

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Conrad, Jan, et Olaf Reimer. « Indirect dark matter searches in gamma and cosmic rays ». Nature Physics 13, n^o 3 (mars 2017) : 224–31. http://dx.doi.org/10.1038/nphys4049.

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Demidov, S. V., et O. V. Suvorova. « Indirect searches for dark matter at Baksan and Baikal ». Physics of Particles and Nuclei 46, n^o 2 (mars 2015) : 222–29. http://dx.doi.org/10.1134/s1063779615020070.

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Mahmoudi, Farvah, et Alexandre Arbey. « Complementarity of direct and indirect searches in the pMSSM ». Nuclear and Particle Physics Proceedings 263-264 (juin 2015) : 80–85. http://dx.doi.org/10.1016/j.nuclphysbps.2015.04.015.

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Palacio, J., D. Navarro-Girones et J. Rico. « Pointing optimization for IACTs on indirect dark matter searches ». Astroparticle Physics 104 (janvier 2019) : 84–90. http://dx.doi.org/10.1016/j.astropartphys.2018.09.002.

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Gaskins, Jennifer M. « A review of indirect searches for particle dark matter ». Contemporary Physics 57, n^o 4 (7 juin 2016) : 496–525. http://dx.doi.org/10.1080/00107514.2016.1175160.

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Vivier, M. « Recent results on indirect dark matter searches with H.E.S.S. » EAS Publications Series 36 (2009) : 291–95. http://dx.doi.org/10.1051/eas/0936041.

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DREINER, H., J. ELLIS, D. V. NANOPOULOS, N. D. TRACAS et N. D. VLACHOS. « INDIRECT SEARCHES FOR LEPTOQUARKS AT PRESENT AND FUTURE COLLIDERS ». Modern Physics Letters A 03, n^o 04 (mars 1988) : 443–50. http://dx.doi.org/10.1142/s0217732388000520.

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We explore the sensitivities of e+e− colliders (LEP, CLIC) and hadron-hadron colliders (CERN [Formula: see text], FNAL [Formula: see text], LHC pp and SSC pp) to the indirect effects of virtual scalar particles with superstring-inspired leptoquark and diquark couplings. We find that e+e− colliders have better sensitivities via total cross section measurements of [Formula: see text] than via asymmetry measurements, and that LEP 2 is much more sensitive than LEP 1. Hadron-hadron colliders are sensitive via lepton-pair production cross sections ( [Formula: see text]μ+μ−, τ+τ−).

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Argüelles, Carlos A., et Joachim Kopp. « Sterile neutrinos and indirect dark matter searches in IceCube ». Journal of Cosmology and Astroparticle Physics 2012, n^o 07 (6 juillet 2012) : 016. http://dx.doi.org/10.1088/1475-7516/2012/07/016.

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Bigi, I. I., et S. Wakaizumi. « Indirect searches for ultra-heavy quarks in rare decays ». Physics Letters B 188, n^o 4 (avril 1987) : 501–5. http://dx.doi.org/10.1016/0370-2693(87)91657-1.

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41

Funk, Stefan. « Indirect detection of dark matter with γ rays ». Proceedings of the National Academy of Sciences 112, n^o 40 (12 mai 2014) : 12264–71. http://dx.doi.org/10.1073/pnas.1308728111.

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The details of what constitutes the majority of the mass that makes up dark matter in the Universe remains one of the prime puzzles of cosmology and particle physics today—80 y after the first observational indications. Today, it is widely accepted that dark matter exists and that it is very likely composed of elementary particles, which are weakly interacting and massive [weakly interacting massive particles (WIMPs)]. As important as dark matter is in our understanding of cosmology, the detection of these particles has thus far been elusive. Their primary properties such as mass and interaction cross sections are still unknown. Indirect detection searches for the products of WIMP annihilation or decay. This is generally done through observations of γ-ray photons or cosmic rays. Instruments such as the Fermi large-area telescope, high-energy stereoscopic system, major atmospheric gamma-ray imaging Cherenkov, and very energetic radiation imaging telescope array, combined with the future Cherenkov telescope array, will provide important complementarity to other search techniques. Given the expected sensitivities of all search techniques, we are at a stage where the WIMP scenario is facing stringent tests, and it can be expected that WIMPs will be either be detected or the scenario will be so severely constrained that it will have to be rethought. In this sense, we are on the threshold of discovery. In this article, I will give a general overview of the current status and future expectations for indirect searches of dark matter (WIMP) particles.

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Khlopov, Maxim Yu. « Introduction to the special issue on "indirect dark matter searches" ». Modern Physics Letters A 29, n^o 37 (4 décembre 2014) : 1402001. http://dx.doi.org/10.1142/s0217732314020015.

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The nature of cosmological dark matter finds its explanation in physics beyond the Standard Model of elementary particles. The landscape of dark matter candidates contains a wide variety of species, either elusive or hardly detectable in direct experimental searches. Even in case, when such searches are possible the interpretation of their results implies additional sources of information, which provide indirect effects of dark matter. Some nontrivial probes for the nature of the dark matter are presented in the present issue.

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Morselli, Aldo. « Search for dark matter with IACTs and the Cherenkov Telescope Array ». Journal of Physics : Conference Series 2429, n^o 1 (1 février 2023) : 012019. http://dx.doi.org/10.1088/1742-6596/2429/1/012019.

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Abstract In the last decades an incredible amount of evidence for the existence of dark matter (DM) has been accumulating. At the same time, many efforts have been undertaken to try to identify what dark matter is made of. Indirect searches look at places in the Universe where dark matter is known to be abundant and seek for possible annihilation or decay signatures. Indirect searches with the Fermi Gamma ray Space Telescope and Imaging Atmospheric Cherenkov Telescopes (IACTs) are playing a crucial role in constraining the nature of the DM particle through the study of their annihilation into gamma rays from different astrophysical structures. In this talk I will review the status of the search with IACTs and I will describe the sensitivity projections for dark matter searches on the various targets taking into account the latest instrument response functions expected for the Cherenkov Telescope Array (CTA) together with estimations for the systematic uncertainties from diffuse astrophysical and cosmic-ray backgrounds.

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Gaggero, Daniele, et Mauro Valli. « Impact of Cosmic-Ray Physics on Dark Matter Indirect Searches ». Advances in High Energy Physics 2018 (17 décembre 2018) : 1–23. http://dx.doi.org/10.1155/2018/3010514.

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The quest for the elusive dark matter (DM) that permeates the Universe (and in general the search for signatures of physics beyond the Standard Model at astronomical scales) provides a unique opportunity and a tough challenge to the high energy astrophysics community. In particular, the so-called DMindirect searches—mostly focused on a class of theoretically well-motivated DM candidates such as the weakly interacting massive particles—are affected by a complex astrophysical background of cosmic radiation. The understanding and modeling of such background require a deep comprehension of an intricate classical plasma physics problem, i.e., the interaction between high energy charged particles, accelerated in peculiar astrophysical environments, and magnetohydrodynamic turbulence in the interstellar medium of our galaxy. In this review we highlight several aspects of this exciting interplay between the most recent claims of DM annihilation/decay signatures from the sky and the galactic cosmic-ray research field. Our purpose is to further stimulate the debate about viable astrophysical explanations, discussing possible directions that would help breaking degeneracy patterns in the interpretation of current data. We eventually aim to emphasize how a deep knowledge on the physics of CR transport is therefore required to tackle the DM indirect search program at present and in the forthcoming years.

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Beck, Geoff. « Radio-Frequency Searches for Dark Matter in Dwarf Galaxies ». Galaxies 7, n^o 1 (13 janvier 2019) : 16. http://dx.doi.org/10.3390/galaxies7010016.

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Dwarf spheroidal galaxies have long been discussed as optimal targets for indirect dark matter searches. However, the majority of such studies have been conducted with gamma-ray instruments. In this review, we discuss the very recent progress that has been made in radio-based indirect dark matter searches. We look at existing work on this topic and discuss the future prospects that motivate continued work in this newly developing field that promises to become, in the light of the up-coming Square Kilometre Array, a prominent component of the hunt for dark matter.

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Calore, Francesca, Nassim Bozorgnia, Mark Lovell, Gianfranco Bertone, Matthieu Schaller, Carlos S. Frenk, Robert A. Crain, Joop Schaye, Tom Theuns et James W. Trayford. « Simulated Milky Way analogues : implications for dark matter indirect searches ». Journal of Cosmology and Astroparticle Physics 2015, n^o 12 (29 décembre 2015) : 053. http://dx.doi.org/10.1088/1475-7516/2015/12/053.

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Mazziotta, M. N. « Indirect searches for dark matter with the Fermi LAT instrument ». International Journal of Modern Physics A 29, n^o 22 (29 août 2014) : 1430030. http://dx.doi.org/10.1142/s0217751x14300300.

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In this review the current status of several searches for particle dark matter with the Fermi Large Area Telescope instrument is presented. In particular, the current limits on the weakly interacting massive particles, obtained from the analyses of gamma-ray and cosmic ray electron/positron data, will be illustrated.

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Fornengo, Nicolao. « Status and perspectives of indirect and direct dark matter searches ». Advances in Space Research 41, n^o 12 (janvier 2008) : 2010–18. http://dx.doi.org/10.1016/j.asr.2007.02.067.

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Ando, Shin'ichiro, Bradley J. Kavanagh, Oscar Macias, Tiago Alves, Siebren Broersen, Stijn Delnoij, Thomas Goldman et al. « Discovery prospects of dwarf spheroidal galaxies for indirect dark matter searches ». Journal of Cosmology and Astroparticle Physics 2019, n^o 10 (14 octobre 2019) : 040. http://dx.doi.org/10.1088/1475-7516/2019/10/040.

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Albert, Andrea. « Indirect Searches for Dark Matter with the Fermi Large Area Telescope1 ». Physics Procedia 61 (2015) : 6–12. http://dx.doi.org/10.1016/j.phpro.2014.12.004.

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