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Автор: Grafiati

Опубліковано: 7 вересня 2023

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1

Feder, Toni. "Dark-matter searches." Physics Today 67, no. 9 (September 2014): 25. http://dx.doi.org/10.1063/pt.3.2513.

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2

SADOULET, BERNARD. "DARK MATTER SEARCHES." International Journal of Modern Physics A 15, supp01b (July 2000): 687–714. http://dx.doi.org/10.1142/s0217751x00005371.

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3

Pretzl, K. "Dark Matter Searches." Space Science Reviews 130, no. 1-4 (March 23, 2007): 63–72. http://dx.doi.org/10.1007/s11214-007-9151-0.

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4

BAUDIS, LAURA. "DARK MATTER SEARCHES." International Journal of Modern Physics A 21, no. 08n09 (April 10, 2006): 1925–37. http://dx.doi.org/10.1142/s0217751x06032873.

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Анотація:

More than 90% of matter in the Universe could be composed of heavy particles, which were non-relativistic, or 'cold', when they froze-out from the primordial soup. I will review current searches for these hypothetical particles, both via interactions with nuclei in deep underground detectors, and via the observation of their annihilation products in the Sun, galactic halo and galactic center.

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5

Baudis, Laura. "Dark matter searches." Annalen der Physik 528, no. 1-2 (July 31, 2015): 74–83. http://dx.doi.org/10.1002/andp.201500114.

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6

Baudis, Laura. "Cryogenic Dark Matter Searches." Europhysics News 52, no. 3 (2021): 22–24. http://dx.doi.org/10.1051/epn/2021304.

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In the decades-old quest to uncover the nature of the enigmatic dark matter, cryogenic detectors have reached unprecedented sensitivities. Searching for tiny signals from dark matter particles scattering in materials cooled down to low temperatures, these experiments look out into space from deep underground. Their ambitious goal is to discover non-gravitational interactions of dark matter and to scan the allowed parameter space until interactions from solar and cosmic neutrinos are poised to take over.

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7

J. C. Spooner, Neil. "Direct Dark Matter Searches." Journal of the Physical Society of Japan 76, no. 11 (November 15, 2007): 111016. http://dx.doi.org/10.1143/jpsj.76.111016.

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8

Seidel, Wolfgang. "Cryogenic dark matter searches." Nuclear Physics B - Proceedings Supplements 138 (January 2005): 130–34. http://dx.doi.org/10.1016/j.nuclphysbps.2004.11.031.

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9

Gascon, J. "Direct Dark Matter Searches." Nuclear Physics B - Proceedings Supplements 143 (June 2005): 423–28. http://dx.doi.org/10.1016/j.nuclphysbps.2005.01.139.

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10

Gelmini, G. B., P. Gondolo, and E. Roulet. "Neutralino dark matter searches." Nuclear Physics B 351, no. 3 (March 1991): 623–44. http://dx.doi.org/10.1016/s0550-3213(05)80036-7.

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11

Spiro, Michel, Éric Aubourg, and Nathalie Palanque-Delabrouille. "Searches for dark matter." Nuclear Physics B - Proceedings Supplements 80, no. 1-3 (January 2000): 95–107. http://dx.doi.org/10.1016/s0920-5632(99)00832-4.

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12

Gascon, J. "Dark Matter direct searches." Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 520, no. 1-3 (March 2004): 96–100. http://dx.doi.org/10.1016/j.nima.2003.11.251.

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13

Sadoulet, B. "Searches for dark matter." Nuclear Physics B - Proceedings Supplements 35 (May 1994): 117–27. http://dx.doi.org/10.1016/0920-5632(94)90229-1.

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14

KHLOPOV, M. Y., A. G. MAYOROV, and E. Y. SOLDATOV. "COMPOSITE DARK MATTER AND PUZZLES OF DARK MATTER SEARCHES." International Journal of Modern Physics D 19, no. 08n10 (August 2010): 1385–95. http://dx.doi.org/10.1142/s0218271810017962.

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Анотація:

Positive results of dark matter searches in DAMA/ NaI and DAMA/LIBRA experiments, being put together with the results of other groups, can imply nontrivial particle physics solutions for cosmological dark matter. Stable particles with charge -2, bound with primordial helium in O -helium "atoms" ( OHe ), represent a specific warmer than cold nuclear-interacting form of dark matter. Slowed down in the terrestrial matter, OHe is elusive for direct methods of underground dark matter detection used in cryogenic experiments. However the radiative capture of OHe by Na and I nuclei can lead to annual variations of energy release in the energy interval of 2–5 keV in DAMA/ NaI and DAMA/LIBRA experiments.

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15

Rosenberg, Leslie J. "Dark-matter QCD-axion searches." Proceedings of the National Academy of Sciences 112, no. 40 (January 12, 2015): 12278–81. http://dx.doi.org/10.1073/pnas.1308788112.

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Анотація:

In the late 20th century, cosmology became a precision science. Now, at the beginning of the next century, the parameters describing how our universe evolved from the Big Bang are generally known to a few percent. One key parameter is the total mass density of the universe. Normal matter constitutes only a small fraction of the total mass density. Observations suggest this additional mass, the dark matter, is cold (that is, moving nonrelativistically in the early universe) and interacts feebly if at all with normal matter and radiation. There’s no known such elementary particle, so the strong presumption is the dark matter consists of particle relics of a new kind left over from the Big Bang. One of the most important questions in science is the nature of this dark matter. One attractive particle dark-matter candidate is the axion. The axion is a hypothetical elementary particle arising in a simple and elegant extension to the standard model of particle physics that nulls otherwise observable CP-violating effects (where CP is the product of charge reversal C and parity inversion P) in quantum chromo dynamics (QCD). A light axion of mass 10−(6–3) eV (the invisible axion) would couple extraordinarily weakly to normal matter and radiation and would therefore be extremely difficult to detect in the laboratory. However, such an axion is a compelling dark-matter candidate and is therefore a target of a number of searches. Compared with other particle dark-matter candidates, the plausible range of axion dark-matter couplings and masses is narrowly constrained. This focused search range allows for definitive searches, where a nonobservation would seriously impugn the dark-matter QCD-axion hypothesis. Axion searches use a wide range of technologies, and the experiment sensitivities are now reaching likely dark-matter axion couplings and masses. This article is a selective overview of the current generation of sensitive axion searches. Not all techniques and experiments are discussed, but I hope to give a sense of the current experimental landscape of the search for dark-matter axions.

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16

Boveia, Antonio, and Caterina Doglioni. "Dark Matter Searches at Colliders." Annual Review of Nuclear and Particle Science 68, no. 1 (October 19, 2018): 429–59. http://dx.doi.org/10.1146/annurev-nucl-101917-021008.

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Анотація:

Colliders, among the most successful tools of particle physics, have revealed much about matter. This review describes how colliders contribute to the search for particle dark matter, focusing on the highest-energy collider currently in operation, the Large Hadron Collider (LHC) at CERN. In the absence of hints about the character of interactions between dark matter and standard matter, this review emphasizes what could be observed in the near future, presents the main experimental challenges, and discusses how collider searches fit into the broader field of dark matter searches. Finally, it highlights a few areas to watch for the future LHC program.

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17

Khlopov, Maxim. "Dark atoms and puzzles of dark matter searches." International Journal of Modern Physics A 29, no. 19 (July 30, 2014): 1443002. http://dx.doi.org/10.1142/s0217751x14430027.

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Анотація:

The nonbaryonic dark matter of the universe is assumed to consist of new stable forms of matter. Their stability reflects symmetry of micro world and particle candidates for cosmological dark matter are the lightest particles that bear new conserved quantum numbers. Dark matter candidates can appear in the new families of quarks and leptons and the existence of new stable charged leptons and quarks is possible, if they are hidden in elusive "dark atoms." Such possibility, strongly restricted by the constraints on anomalous isotopes of light elements, is not excluded in scenarios that predict stable double charged particles. The excessive -2 charged particles are bound in these scenarios with primordial helium in O -helium "atoms," maintaining specific nuclear-interacting form of the dark matter, which may provide an interesting solution for the puzzles of the direct dark matter searches.

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18

Cebrián, Susana. "Review on dark matter searches." Journal of Physics: Conference Series 2502, no. 1 (May 1, 2023): 012004. http://dx.doi.org/10.1088/1742-6596/2502/1/012004.

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Abstract Dark matter particles populating our galactic halo could be directly detected by measuring their scattering off target nuclei or electrons in a suitable detector. As this interaction is expected to occur with very low probability and would generate very small energy deposits, the detection is challenging; the possible identification of distinctive signatures (like an annual modulation in the interaction rates or directionality) to assign a dark matter origin to a possible observation is being considered. Here, the physics case of different dark matter direct detection experiments will be presented and the different and complementary techniques which are being applied or considered will be discussed, summarizing their features and latest results obtained. Special focus will be made on TPC-related projects; experiments using noble liquids have presently a leading role to constrain interaction cross sections of a wide range of dark matter candidates and gaseous detectors are very promising to explore specifically low mass dark matter as well as to measure directionality.

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19

Gatti, Claudio, Paola Gianotti, Carlo Ligi, Mauro Raggi, and Paolo Valente. "Dark Matter Searches at LNF." Universe 7, no. 7 (July 9, 2021): 236. http://dx.doi.org/10.3390/universe7070236.

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Анотація:

In recent years, the absence of experimental evidence for searches dedicated to dark matter has triggered the development of new ideas on the nature of this entity, which manifests at the cosmological level. Some of these can be explored by small experiments with a short timescale and an investment that can be afforded by national laboratories, such as the Frascati one. This is the main reason why a laboratory that, traditionally, was focused in particle physics studies with accelerators has begun intense activity in this field of research.

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20

Georgescu, Iulia. "Quantum searches for dark matter." Nature Reviews Physics 4, no. 4 (March 11, 2022): 216. http://dx.doi.org/10.1038/s42254-022-00442-6.

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21

Casanellas, Jordi. "Dark matter searches with asteroseismology." EPJ Web of Conferences 101 (2015): 01015. http://dx.doi.org/10.1051/epjconf/201510101015.

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22

Gascon, Jules. "Direct dark matter searches review." EPJ Web of Conferences 95 (2015): 02004. http://dx.doi.org/10.1051/epjconf/20159502004.

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23

Mosca, Luigi. "Experimental searches for Dark Matter." Surveys in High Energy Physics 9, no. 2-4 (April 1996): 275–305. http://dx.doi.org/10.1080/01422419608223782.

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24

Tao, C. "Dark Matter searches: an overview." Journal of Instrumentation 15, no. 06 (June 25, 2020): C06054. http://dx.doi.org/10.1088/1748-0221/15/06/c06054.

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25

Mitsou, Vasiliki A. "Dark matter searches at LHC." Journal of Physics: Conference Series 335 (December 28, 2011): 012003. http://dx.doi.org/10.1088/1742-6596/335/1/012003.

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26

Cao, Zheng. "Dark Matter: Candidates and Searches." Journal of Physics: Conference Series 1634 (September 2020): 012158. http://dx.doi.org/10.1088/1742-6596/1634/1/012158.

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27

Sadoulet, Bernard. "Direct searches for dark matter." Nuclear Physics B - Proceedings Supplements 77, no. 1-3 (May 1999): 389–97. http://dx.doi.org/10.1016/s0920-5632(99)00448-x.

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28

Barish, Barry C. "Indirect searches for dark matter." Nuclear Physics B - Proceedings Supplements 77, no. 1-3 (May 1999): 398–401. http://dx.doi.org/10.1016/s0920-5632(99)00449-1.

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29

Fornengo, N. "Supersymmetric dark matter — direct searches." Nuclear Physics B - Proceedings Supplements 81 (February 2000): 30–36. http://dx.doi.org/10.1016/s0920-5632(99)00854-3.

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30

Brun, Pierre, Jean-François Glicenstein, Emmanuel Moulin, and Matthieu Vivier. "Dark matter searches with H.E.S.S." Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 630, no. 1 (February 2011): 151–54. http://dx.doi.org/10.1016/j.nima.2010.06.049.

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31

Nuss, E. "Dark Matter searches with GLAST." Advances in Space Research 41, no. 12 (January 2008): 2029–31. http://dx.doi.org/10.1016/j.asr.2007.03.045.

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32

CIRELLI, MARCO. "Indirect searches for dark matter." Pramana 79, no. 5 (October 27, 2012): 1021–43. http://dx.doi.org/10.1007/s12043-012-0419-x.

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33

Strigari, Louis E. "Galactic searches for dark matter." Physics Reports 531, no. 1 (October 2013): 1–88. http://dx.doi.org/10.1016/j.physrep.2013.05.004.

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34

Rosenberg, Leslie J. "Dark-matter QCD-axion searches." Journal of Physics: Conference Series 203 (January 1, 2010): 012008. http://dx.doi.org/10.1088/1742-6596/203/1/012008.

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35

Daci, Nadir. "Dark matter searches in CMS." Journal of Physics: Conference Series 623 (June 11, 2015): 012029. http://dx.doi.org/10.1088/1742-6596/623/1/012029.

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36

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

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37

Kahlhoefer, Felix. "Review of LHC dark matter searches." International Journal of Modern Physics A 32, no. 13 (May 5, 2017): 1730006. http://dx.doi.org/10.1142/s0217751x1730006x.

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Анотація:

This review discusses both experimental and theoretical aspects of searches for dark matter at the LHC. An overview of the various experimental search channels is given, followed by a summary of the different theoretical approaches for predicting dark matter signals. A special emphasis is placed on the interplay between LHC dark matter searches and other kinds of dark matter experiments, as well as among different types of LHC searches.

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38

Behr, J. Katharina, and Alexander Grohsjean. "Dark Matter Searches with Top Quarks." Universe 9, no. 1 (December 27, 2022): 16. http://dx.doi.org/10.3390/universe9010016.

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Анотація:

Collider signatures with top quarks provide sensitive probes of dark matter (DM) production at the Large Hadron Collider (LHC). In this article, we review the results of DM searches in final states with top quarks conducted by the ATLAS and CMS Collaborations at the LHC, including the most recent results on the full LHC Run 2 dataset. We highlight the complementarity of DM searches in final states with top quarks with searches in other final states in the framework of various simplified models of DM. A reinterpretation of a DM search with top quarks in the context of an effective field theory description of scalar dark energy is also discussed. Finally, we give an outlook on the potential of DM searches with top quarks in LHC Run 3, at the high-luminosity LHC, and possible future colliders. In this context, we highlight new benchmark models that could be probed by existing and future searches as well as those that predict still-uncovered signatures of anomalous top-quark production and decays at the LHC.

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39

IBARRA, ALEJANDRO, DAVID TRAN, and CHRISTOPH WENIGER. "INDIRECT SEARCHES FOR DECAYING DARK MATTER." International Journal of Modern Physics A 28, no. 27 (October 30, 2013): 1330040. http://dx.doi.org/10.1142/s0217751x13300408.

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Анотація:

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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40

Morgante, Enrico. "Simplified Dark Matter Models." Advances in High Energy Physics 2018 (December 17, 2018): 1–13. http://dx.doi.org/10.1155/2018/5012043.

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I review the construction of simplified models for dark matter searches. After discussing the philosophy and some simple examples, I turn the attention to the aspect of the theoretical consistency and to the implications of the necessary extensions of these models.

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41

Amaro, Fernando Domingues, Elisabetta Baracchini, Luigi Benussi, Stefano Bianco, Cesidio Capoccia, Michele Caponero, Gianluca Cavoto, et al. "Directional Dark Matter Searches with CYGNO." Particles 4, no. 3 (July 6, 2021): 343–53. http://dx.doi.org/10.3390/particles4030029.

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Анотація:

The CYGNO project aims at developing a high resolution Time Projection Chamber with optical readout for directional dark matter searches and solar neutrino spectroscopy. Peculiar CYGNO’s features are the 3D tracking capability provided by the combination of photomultipliers and scientific CMOS camera signals, combined with a helium-fluorine-based gas mixture at atmospheric pressure amplified by gas electron multipliers structures. In this paper, the performances achieved with CYGNO prototypes and the prospects for the upcoming underground installation at Laboratori Nazionali del Gran Sasso of a 50-L detector in fall 2021 will be discussed, together with the plans for a 1-m3 experiment. The synergy with the ERC consolidator, grant project INITIUM, aimed at realising negative ion drift operation within the CYGNO 3D optical approach, will be further illustrated.

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42

Manuel, Bou-Cabo, Ardid Miguel, and Felis Ivan. "Dark matter searches using superheated liquids." EPJ Web of Conferences 121 (2016): 06007. http://dx.doi.org/10.1051/epjconf/201612106007.

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43

Sumner, Timothy J. "Direct dark matter searches - recent highlights." Journal of Physics: Conference Series 312, no. 7 (September 23, 2011): 072003. http://dx.doi.org/10.1088/1742-6596/312/7/072003.

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44

Cerdonio, Massimo, Roberto De Pietri, Philippe Jetzer, and Mauro Sereno. "Local dark matter searches with LISA." Classical and Quantum Gravity 26, no. 9 (April 20, 2009): 094022. http://dx.doi.org/10.1088/0264-9381/26/9/094022.

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45

Porter, Troy A., Robert P. Johnson, and Peter W. Graham. "Dark Matter Searches with Astroparticle Data." Annual Review of Astronomy and Astrophysics 49, no. 1 (September 22, 2011): 155–94. http://dx.doi.org/10.1146/annurev-astro-081710-102528.

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46

Grefe, Michael. "Indirect searches for gravitino dark matter." Journal of Physics: Conference Series 375, no. 1 (July 30, 2012): 012035. http://dx.doi.org/10.1088/1742-6596/375/1/012035.

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47

Taoso, Marco. "Dark matter searches with radio observations." Journal of Physics: Conference Series 485 (March 24, 2014): 012031. http://dx.doi.org/10.1088/1742-6596/485/1/012031.

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48

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

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49

Mijakowski, Piotr. "Dark Matter Searches at Super-Kamiokande." Journal of Physics: Conference Series 1342 (January 2020): 012075. http://dx.doi.org/10.1088/1742-6596/1342/1/012075.

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50

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

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