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Relevant bibliographies by topics / Dark Matter Models

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Academic literature on the topic 'Dark Matter Models'

Author: Grafiati

Published: 18 May 2024

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Journal articles on the topic "Dark Matter Models"

1

Takibayev, N. "Models of dark particle interactions with ordinary matter." Physical Sciences and Technology 2, no. 2 (2015): 58–69. http://dx.doi.org/10.26577/2409-6121-2015-2-2-58-69.

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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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Arnowitt, R., B. Dutta, and Y. Santoso. "Dark matter in Susy models." Physics of Atomic Nuclei 65, no. 12 (2002): 2218–24. http://dx.doi.org/10.1134/1.1530303.

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Arnowitt, R., and Pran Nath. "Models of particle dark matter." Nuclear Physics B - Proceedings Supplements 51, no. 2 (1996): 171–77. http://dx.doi.org/10.1016/s0920-5632(96)00501-4.

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Blinnikov, Sergei I. "Mirror matter and other dark matter models." Uspekhi Fizicheskih Nauk 184, no. 2 (2014): 194–99. http://dx.doi.org/10.3367/ufnr.0184.201402h.0194.

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Blinnikov, S. I. "Mirror matter and other dark matter models." Physics-Uspekhi 57, no. 2 (2014): 183–88. http://dx.doi.org/10.3367/ufne.0184.201402h.0194.

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Feng, Haoyang. "Integrated study of dark matter and dark energy models." Theoretical and Natural Science 34, no. 1 (2024): 162–71. http://dx.doi.org/10.54254/2753-8818/34/20241173.

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Dark matter and dark energy are used as two important concepts in cosmology to explain some of the observed phenomena in the universe. Dark matter is one of the most dominant constituents of the Universe, and it influences the structural formation of the Universe through gravity, including the formation and evolution of galaxies, clusters, and the large-scale structure of the Universe. Dark energy is believed to be one of the causes of the accelerated expansion of the Universe, and its presence explains the observed phenomenon of the accelerating rate of expansion of the Universe. Although the

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Bertacca, Daniele, Nicola Bartolo, and Sabino Matarrese. "Unified Dark Matter Scalar Field Models." Advances in Astronomy 2010 (2010): 1–29. http://dx.doi.org/10.1155/2010/904379.

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We analyze and review cosmological models in which the dynamics of a single scalar field accounts for a unified description of the Dark Matter and Dark Energy sectors, dubbed Unified Dark Matter (UDM) models. In this framework, we consider the general Lagrangian of -essence, which allows to find solutions around which the scalar field describes the desired mixture of Dark Matter and Dark Energy. We also discuss static and spherically symmetric solutions of Einstein's equations for a scalar field with noncanonical kinetic term, in connection with galactic halo rotation curves.

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Boyle, Latham A., Robert R. Caldwell, and Marc Kamionkowski. "Spintessence! New models for dark matter and dark energy." Physics Letters B 545, no. 1-2 (2002): 17–22. http://dx.doi.org/10.1016/s0370-2693(02)02590-x.

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Sussman, Roberto A., Israel Quiros, and Osmel Martín González. "Inhomogeneous models of interacting dark matter and dark energy." General Relativity and Gravitation 37, no. 12 (2005): 2117–43. http://dx.doi.org/10.1007/s10714-005-0199-4.

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Dissertations / Theses on the topic "Dark Matter Models"

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Fedotova, Veronika. "Constraining leptophilic dark matter with KM3NeT." Master's thesis, Alma Mater Studiorum - Università di Bologna, 2021. http://amslaurea.unibo.it/23181/.

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Revealing the nature of the dark matter is among the most puzzling issues of today particle physics, astrophysics and cosmology. Given the striking evidences for dark matter at all astrophysical scales, starting from galactic and going to cosmological scales, a widespread and well motivated assumption on the nature of the dark matter is that it is made by a new particle that extends the Standard Models of Particle Physics. Indirect detection of dark matter, which annihilates in over-dense regions like the galactic centre, is an important probe of a possible dark matter interaction with

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Mantani, Luca. "Simplified t-channel models for dark matter searches." Master's thesis, Alma Mater Studiorum - Università di Bologna, 2017. http://amslaurea.unibo.it/13444/.

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Una enorme quantità di evidenze sperimentali sulla esistenza di una forma di materia non luminosa nell'Universo, si sono accumulate nel corso di circa un secolo. Chiarire la sua natura è diventata una delle sfide più eccitanti ed urgenti negli sforzi per capire il nostro Universo. In questo lavoro presento uno studio su un approccio per scoprire la Materia Oscura interpretata come particella elementare e sulla possibilità di produrla e rilevarla negli acceleratori. Nella parte introduttiva presento una breve storia delle evidenze astrofisiche e astronomiche che hanno portato alla ipotesi del

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PODO, ALESSANDRO. "Topics in composite models and dark matter phenomenology." Doctoral thesis, Scuola Normale Superiore, 2020. http://hdl.handle.net/11384/91400.

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We investigate models of composite dark matter in which the dark matter candidate arises naturally as an accidentally stable bound state of a confining dynamics and with observable signatures in a wide variety of experiments. In the first part of the thesis we introduce and explore a new class of models with dark fermions in the adjoint repre- sentation of the confining gauge group. The low energy dynamics and the cosmological history are peculiar and provide a dark matter candidate with properties much different from that of a canonical WIMP. The dark matter is heavy but has a large interacti

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Biondi, Federico. "formation of dark matter haloes: models and simulations." Doctoral thesis, Università degli studi di Padova, 2010. http://hdl.handle.net/11577/3426888.

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At present, the best model for the Universe as a whole is given by the so called ``Hot Big Bang'', which describes an expanding universe in which the density and temperature of matter and radiation are followed in time. The value of the parameters characterizing the observed universe is summarized by the concordance $\Lambda$CDM model, where CDM stands for Cold Dark Matter (the main matter component), and $\Lambda$ is the cosmological constant (some kind of unknown energy, with an anti-gravitational effect). According to this model, the universe is spatially flat (i.e. the density parameter $\

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Zsembinszki, Gabriel. "Light scalar fields in a dark universe: models of inflation, dark energy and dark matter." Doctoral thesis, Universitat Autònoma de Barcelona, 2007. http://hdl.handle.net/10803/3390.

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La teoría científica de más éxito hoy en día, sobre el origen y la evolución del universo, es conocida como el modelo estándar del Big Bang, el cual es una de las construcciones intelectuales más ambiciosas de la humanidad. Se basa en dos ramas bien consolidadas de la física teórica, a saber, la teoría de la Relatividad General y el Modelo Estándar de la física de partículas, y es capaz de hacer predicciones sólidas, como la expansión del universo, la existencia del fondo de radiación de microondas y las abundancias relativas de los elementos ligeros. Algunas de las predicciones teóricas ya ha

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Costa, André Alencar da. "Observational Constraints on Models with an Interaction between Dark Energy and Dark Matter." Universidade de São Paulo, 2014. http://www.teses.usp.br/teses/disponiveis/43/43134/tde-20012015-123002/.

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In this thesis we go beyond the standard cosmological LCDM model and study the effect of an interaction between dark matter and dark energy. Although the LCDM model provides good agreement with observations, it faces severe challenges from a theoretical point of view. In order to solve such problems, we first consider an alternative model where both dark matter and dark energy are described by fluids with a phenomenological interaction given by a combination of their energy densities. In addition to this model, we propose a more realistic one based on a Lagrangian density with a Yukawa-type in

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Kast, Simon Florian [Verfasser], and U. [Akademischer Betreuer] Nierste. "Dark Matter from the Top - Simplified Models of Flavoured Dark Matter in Dark Minimal Flavour Violation / Simon Florian Kast ; Betreuer: U. Nierste." Karlsruhe : KIT-Bibliothek, 2017. http://d-nb.info/1147485143/34.

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Le, Delliou Morgan. "Self-similar infall models for cold dark matter haloes." Thesis, National Library of Canada = Bibliothèque nationale du Canada, 2002. http://www.collectionscanada.ca/obj/s4/f2/dsk3/ftp05/NQ63431.pdf.

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Sotelo, Denis Stefan Robertson. "Probing Self-Interacting Dark Matter Models with Neutrino Telescopes." Universidade de São Paulo, 2017. http://www.teses.usp.br/teses/disponiveis/43/43134/tde-25012018-015636/.

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In this thesis we studied dark matter models with strong self-interactions, typically known as self-interacting dark matter (SIDM). This kind of models constitute a promising solution to the tension between small scale structure observations and predictions assuming the standard case of collisionless cold dark matter (CDM) while keeping the success of the standard cosmological model, LambdaCDM, at large scales. The presence of strong self-interactions can increase the dark matter capture and annihilation in astrophysical objects like our sun, enhancing the potential of indirect detection signa

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Mead, Alexander James. "Demographics of dark-matter haloes in standard and non-standard cosmologies." Thesis, University of Edinburgh, 2014. http://hdl.handle.net/1842/9951.

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This thesis explores topics related to the formation and development of the large-scale structure in the Universe, with the focus being to compute properties of the evolved non-linear density field in an approximate way. The first three chapters form an introduction: Chapter 1 contains the theoretical basis of modern cosmology, Chapter 2 discusses the role of N-body simulations in the study of structure formation and Chapter 3 considers the phenomenological halo model. In Chapter 4 a novel method of computing the matter power spectrum is developed. This method uses the halo model directly to m

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Books on the topic "Dark Matter Models"

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

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

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Schramm, David N. Probing the big bang with LEP. Fermi National Accelerator Laboratory, 1990.

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1952-, Sanchez N., and Zichichi Antonino, eds. Advances in astrofundamental physics: International School of Astrophysics "D Chalonge" : Erice, Italy, 1994. World Scientific, 1995.

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United States. National Aeronautics and Space Administration., ed. Final technical report: Studies of the evolution of the X-ray emission of clusters of galaxies. National Aeronautics and Space Administration, 1990.

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United States. National Aeronautics and Space Administration., ed. Final technical report: Studies of the evolution of the X-ray emission of clusters of galaxies. National Aeronautics and Space Administration, 1990.

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1964-, Kelly Karen J., Schröder Barbara 1969-, Vandecaveye Giel, Fundação de Serralves (Portugal), Stedelijk Museum voor Actuele Kunst (Ghent, Belgium), and Museu Serralves, eds. Dara Birnbaum: The dark matter of media light. S.M.A.K., 2010.

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Prime elements of ordinary matter, dark matter & dark energy: Beyond standard model & string theory. 2nd ed. Universal Publishers, 2007.

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Dark matter: Art and politics in the age of enterprise culture. PlutoPress, 2011.

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E'kov, Evgeniy. The origin and evolution of the Universe. INFRA-M Academic Publishing LLC., 2022. http://dx.doi.org/10.12737/1852616.

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The monograph examines a wide range of problems related to the origin and development of the Universe. An overview of the history of the study of astronomy from Stone Age observatories to modern space telescopes is given. The theories of the origin of the Universe are analyzed, evidence of the Big Bang, the expansion of the Universe, the cosmic effects of dark energy and dark matter are given. The origin and causes of the existence of planets, stars, nebulae, galaxies and other cosmic bodies in the Universe are considered. A large place is given to the analysis of the origin and development of

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Book chapters on the topic "Dark Matter Models"

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Rowan-Robinson, M., and J. Crawford. "Models for IRAS Galaxies." In Light on Dark Matter. Springer Netherlands, 1986. http://dx.doi.org/10.1007/978-94-009-4672-9_89.

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Beckman, John E. "Constraints on Baryon-Dominated Cosmological Models from Light Element Abundances and CMB Fluctuations." In Baryonic Dark Matter. Springer Netherlands, 1990. http://dx.doi.org/10.1007/978-94-009-0565-8_16.

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Bauer, Martin, and Tilman Plehn. "WIMP Models." In Yet Another Introduction to Dark Matter. Springer International Publishing, 2019. http://dx.doi.org/10.1007/978-3-030-16234-4_4.

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Rowan-Robinson, M., A. Lock, D. W. Walker, and S. Harris. "Models of IRAS Observations of Circumstellar Shells." In Light on Dark Matter. Springer Netherlands, 1986. http://dx.doi.org/10.1007/978-94-009-4672-9_20.

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Crawford, J., and M. Rowan-Robinson. "Models for IRAS Observations of Galactic HII Regions." In Light on Dark Matter. Springer Netherlands, 1986. http://dx.doi.org/10.1007/978-94-009-4672-9_66.

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Sparke, Linda S. "Self-Gravitating Polar Ring Models." In Dark Matter in the Universe. Springer Netherlands, 1987. http://dx.doi.org/10.1007/978-94-009-4772-6_64.

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Martel, Hugo. "Cosmological models with ʌ≠0." In Dark Matter in the Universe. Springer Netherlands, 1990. http://dx.doi.org/10.1007/978-94-009-1940-2_9.

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Larson, Richard B. "Bimodal Star Formation and Remnant-Dominated Galactic Models." In Dark Matter in the Universe. Springer Netherlands, 1987. http://dx.doi.org/10.1007/978-94-009-4772-6_85.

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Shafi, Q. "Particle Physics and Cosmology Beyond the Standard Model(S): Grand Unification and Three Generation Superstring Models." In Dark Matter in the Universe. Springer Netherlands, 1990. http://dx.doi.org/10.1007/978-94-009-1940-2_4.

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Bianchi, Massimo, Roland Allen, and Antonio Mondragon. "Dark Matter, Supersymmetry and Supergravity Models." In Concise Encyclopedia of Supersymmetry. Springer Netherlands, 2004. http://dx.doi.org/10.1007/1-4020-4522-0_148.

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Conference papers on the topic "Dark Matter Models"

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Wambsganss, Joachim, Renyue Cen, Jeremiah P. Ostriker, and Edwin L. Turner. "Testing cosmogonic models with gravitational lensing." In Dark matter. AIP, 1995. http://dx.doi.org/10.1063/1.48356.

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Lavalle, Julien. "Analytical models of dark matter subhalos for indirect dark matter searches." In XVIII International Conference on Topics in Astroparticle and Underground Physics. Sissa Medialab, 2024. http://dx.doi.org/10.22323/1.441.0045.

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Ibe, Masahiro. "Overview on Dark Matter Models." In Proceedings of the 10th International Workshop on Very High Energy Particle Astronomy in 2019 (VHEPA2019). Journal of the Physical Society of Japan, 2023. http://dx.doi.org/10.7566/jpscp.39.011007.

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Lee, Hyun Min, and Min-Seok Seo. "Models for SIMP dark matter and dark photon." In CETUP* 2015 – WORKSHOP ON DARK MATTER, NEUTRINO PHYSICS AND ASTROPHYSICS AND PPC 2015 – IXTH INTERNATIONAL CONFERENCE ON INTERCONNECTIONS BETWEEN PARTICLE PHYSICS AND COSMOLOGY. Author(s), 2016. http://dx.doi.org/10.1063/1.4953320.

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Buyle, Pieter, Herwig Dejonghe, and GIANFRANCO GENTILE. "Beyond the sphericitiy assumption in dynamical HI models." In Baryons in Dark Matter Halos. Sissa Medialab, 2004. http://dx.doi.org/10.22323/1.014.0076.

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D'Auria, John. "New phenomenological constraints for dark matter models in disks." In Baryons in Dark Matter Halos. Sissa Medialab, 2004. http://dx.doi.org/10.22323/1.014.0051.

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BLINNIKOV, S. I. "MIRROR MATTER AND OTHER MODELS FOR DARK MATTER." In Pomeranchuk 100. WORLD SCIENTIFIC, 2014. http://dx.doi.org/10.1142/9789814616850_0002.

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PETER, Annika, Christopher E. Moody, Andrew J. Benson, and Marc Kamionkowski. "Constraints on decaying-dark-matter models from simulations of isolated halos." In Identification of Dark Matter 2010. Sissa Medialab, 2011. http://dx.doi.org/10.22323/1.110.0084.

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Mambrini, Yann. "Building phenomenological models of Dark Matter." In 11th International Workshop Dark Side of the Universe 2015. Sissa Medialab, 2016. http://dx.doi.org/10.22323/1.268.0040.

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Lin, Tongyan. "Dark matter models and direct detection." In Theoretical Advanced Study Institute Summer School 2018 "Theory in an Era of Data". Sissa Medialab, 2019. http://dx.doi.org/10.22323/1.333.0009.

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Reports on the topic "Dark Matter Models"

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Chen, Hui, Winston Wei Dou, and Leonid Kogan. Measuring “Dark Matter” in Asset Pricing Models. National Bureau of Economic Research, 2019. http://dx.doi.org/10.3386/w26418.

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Primulando, Reinard. Dark Matter in the Heavens and at Colliders: Models and Constraints. Office of Scientific and Technical Information (OSTI), 2012. http://dx.doi.org/10.2172/1127918.

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Abdallah, Jalal, Adi Ashkenazi, Antonio Boveia, et al. Simplified Models for Dark Matter and Missing Energy Searches at the LHC. Office of Scientific and Technical Information (OSTI), 2014. http://dx.doi.org/10.2172/1304777.

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Boveia, Antonio, Oliver Buchmueller, Giorgio Busoni, et al. Recommendations on presenting LHC searches for missing transverse energy signals using simplified s-channel models of dark matter. Office of Scientific and Technical Information (OSTI), 2016. http://dx.doi.org/10.2172/1255141.

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Wang, Zhixing. Search for resonance in inclusive and b-tagged dijet mass spectra in proton-proton collision at $\sqrt{s}$ = 13 TeV and constraints on dark matter and other models. Office of Scientific and Technical Information (OSTI), 2020. http://dx.doi.org/10.2172/1764049.

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Krnjaic, Gordan Zdenko. Dark Matter and Color Octets Beyond the Standard Model. Office of Scientific and Technical Information (OSTI), 2012. http://dx.doi.org/10.2172/1127922.

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Chang, Sanghyeon, and Hang Bae Kim. A dark matter solution from the supersymmetric axion model. Office of Scientific and Technical Information (OSTI), 1996. http://dx.doi.org/10.2172/228215.

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Pierce, A. Dark Matter in the Finely Tuned Minimal Supersymmetric Standard Model. Office of Scientific and Technical Information (OSTI), 2004. http://dx.doi.org/10.2172/827002.

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Neogi, Orgho. Search for Dark Matter in a Coannihilation Codex Model With CMS Detector. Office of Scientific and Technical Information (OSTI), 2018. http://dx.doi.org/10.2172/1496031.

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Lisanti, Mariangela, and Jay G. Wacker. Unification and Dark Matter in a Minimal Scalar Extension of the Standard Model. Office of Scientific and Technical Information (OSTI), 2007. http://dx.doi.org/10.2172/902727.

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