Relevant bibliographies by topics / Dark matter

Academic literature on the topic 'Dark matter'

Author: Grafiati
Published: 4 June 2021
Last updated: 31 July 2024

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Journal articles on the topic "Dark matter"

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R K Dubey, R. K. Dubey, Pratima Ojha, and Anil Saini. "Cosmological Model with Dark Energy and Dark Matter." International Journal of Scientific Research 2, no. 5 (June 1, 2012): 400–401. http://dx.doi.org/10.15373/22778179/may2013/135.

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Perković, Dalibor, and Hrvoje Štefančić. "Dark sector unifications: Dark matter-phantom energy, dark matter - constant w dark energy, dark matter-dark energy-dark matter." Physics Letters B 797 (October 2019): 134806. http://dx.doi.org/10.1016/j.physletb.2019.134806.

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Nadar, Arun Kumar Koottharasan. "Exploring the Nature of Dark Matter and Dark Energy." International Journal of Research Publication and Reviews 5, no. 1 (January 24, 2024): 4640–46. http://dx.doi.org/10.55248/gengpi.5.0124.0341.

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Hogan, Craig J. "Dark dark matter." Nature 351, no. 6322 (May 1991): 96–97. http://dx.doi.org/10.1038/351096b0.

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Olive, Keith A. "Dark matter and dark matter candidates." Advances in Space Research 42, no. 3 (August 2008): 581–90. http://dx.doi.org/10.1016/j.asr.2007.07.040.

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Edmonds, Douglas, Duncan Farrah, Djordje Minic, Y. Jack Ng, and Tatsu Takeuchi. "Modified dark matter: Relating dark energy, dark matter and baryonic matter." International Journal of Modern Physics D 27, no. 02 (January 2018): 1830001. http://dx.doi.org/10.1142/s021827181830001x.

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Modified dark matter (MDM) is a phenomenological model of dark matter, inspired by gravitational thermodynamics. For an accelerating universe with positive cosmological constant ([Formula: see text]), such phenomenological considerations lead to the emergence of a critical acceleration parameter related to [Formula: see text]. Such a critical acceleration is an effective phenomenological manifestation of MDM, and it is found in correlations between dark matter and baryonic matter in galaxy rotation curves. The resulting MDM mass profiles, which are sensitive to [Formula: see text], are consistent with observational data at both the galactic and cluster scales. In particular, the same critical acceleration appears both in the galactic and cluster data fits based on MDM. Furthermore, using some robust qualitative arguments, MDM appears to work well on cosmological scales, even though quantitative studies are still lacking. Finally, we comment on certain nonlocal aspects of the quanta of modified dark matter, which may lead to novel nonparticle phenomenology and which may explain why, so far, dark matter detection experiments have failed to detect dark matter particles.
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Poojary, Bhushan. "Dark Matter and Quantum Entanglement Decoded." International Journal of Applied Physics and Mathematics 4, no. 3 (2014): 180–83. http://dx.doi.org/10.7763/ijapm.2014.v4.279.

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Battersby, Stephen. "Dark matter, dark energy, dark… magnetism?" New Scientist 214, no. 2867 (June 2012): 36–39. http://dx.doi.org/10.1016/s0262-4079(12)61430-4.

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de la Macorra, A. "Dark group: dark energy and dark matter." Physics Letters B 585, no. 1-2 (April 2004): 17–23. http://dx.doi.org/10.1016/j.physletb.2004.02.006.

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MORIYAMA, Shigetaka. "Dark Matter." RADIOISOTOPES 63, no. 3 (2014): 151–62. http://dx.doi.org/10.3769/radioisotopes.63.151.

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Dissertations / Theses on the topic "Dark matter"

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Halovanic, Maria. "Dark Matter poems /." College Park, Md. : University of Maryland, 2003. http://hdl.handle.net/1903/110.

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Thesis (M.F.A.) -- University of Maryland, College Park, 2003.
Thesis research directed by: Creative Writing. Title from t.p. of PDF. Includes bibliographical references. Published by UMI Dissertation Services, Ann Arbor, Mich. Also available in paper.
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Zukin, Phillip Gregory. "Dark matter dynamics." Thesis, Massachusetts Institute of Technology, 2012. http://hdl.handle.net/1721.1/77258.

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Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 2012.
This electronic version was submitted by the student author. The certified thesis is available in the Institute Archives and Special Collections.
Cataloged from student-submitted PDF version of thesis.
Includes bibliographical references (p. 147-150).
N-body simulations have revealed a wealth of information about dark matter halos but their results are largely empirical. Here we attempt to shed light on simulation results by using a combination of analytic and numerical methods. First we generalize an analytic model of halo formation, known as Secondary Infall, to include the effects of tidal torque. Given this model we compare its predictions for halo profiles to simulation results and infer that angular momentum plays an important role in setting the structure of dark matter profiles at small radii. Next, we focus on explaining the origin of universality in halos. We find evidence that diffusion -- which can potentially lead to universality -- occurs during halo evolution and is partially sourced by external torques from large scale structure. This is surprising given that the halo is nonlinear and typically thought to be unaffected by neighboring structures. Last, we describe promising ways to analytically describe the evolution of nonlinear halos using a Fokker-Planck formalism.
by Phillip Gregory Zukin.
Ph.D.
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Williams, A. J. R. "Dark matter phenomenology." Thesis, Royal Holloway, University of London, 2013. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.591078.

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In this thesis we present some phenomenological investigations of freeze-in models of dark matter and also a numerical calculation of the particle flux produced by dark matter annihilations around a rotating black hole. Freeze-in is an alternative dark matter production mechanism in which an out of equilibrium very weakly coupled particle is produced in the early universe. We consider the Minimal Supersymmetric Standard Model (MSSM) extended by an additional singlet superfield feebly coupled to the other particles. This feeble coupling leads to a long lifetime for the next to lightest superpartner which can only decay via this coupling. The long lifetime of this decaying particles could lead to displaced vertices which provide a prominent signal for beyond the standard model physics. The phenomenology of the signals from this simple Feebly Interacting Massive Particle (AMP) model is investigated and compared to some experimental searches. The freeze-in mechanism may also constitute an alternative for generating the correct relic density for dark matter candidates whose predicted freeze-out abundance is too low due to a large total annihilation cross section. We show that although such a mechanism could explain why a dark matter candidate has the correct relic density, some candidates may still be ruled out because they would lead to a large gamma ray flux in dwarf spheroidal galaxies or a large elastic scattering rate in direct detection experiments. To investigate this scenario we examine neutralino dark matter in the MSSM. Collisions around black holes may provide a window onto very high energy physics. The geodesics of massless particles produced in collisions near a rotating black hole are solved numerically and a Monte Carlo integration of the momentum distribution of the massless particles is performed to calculate the fraction that escape the black hole to infinity. A distribution of in falling dark matter particles, which are assumed to annihilate to massless panicles, is considered and an estimate of the emergent flux from the collisions is made. The energy spectrum of the emergent particles is found to contain two Lorentz shifted peaks centred on the mass of the dark matter. The separation of the peaks is found to depend on the density profile of the dark matter and could provide information about the size of the annihilation plateau around a black hole and the mass of the dark matter particle.
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Panci, Tibaldo. "Dark matter phenomenology." Paris 7, 2011. http://www.theses.fr/2011PA077061.

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Dans cette thèse j'essaye de résumer la phénoménologie de la Matière Noire (MN) dans tous ses aspects: Détection Directe, Indirecte et constructions de modèles. Il s'agit d'un domaine très prometteur, car la profusion de mesures de ces dernières années l'a rapidement fait progresser et l'a rendu très dynamique. En ce qui concerne la Détection Directe je passe en revue les principaux ingrédients et recettes pour le calcul des signaux dus à une diffusion WIMP-noyau. Je présente le traitement analytique permettant de calculer le taux théorique attendu. Avec un choix standard des caractéristiques du halo de MN et de la section efficace d'interaction, je présente les régions favorisées actuelles et les contraintes sur la MN. En ce qui concerne la Détection Indirecte, je fournis les ingrédients les plus avancés pour calculer les signaux d'annihilations et désintégrations de MN à l'échelle du TeV. Avec ces ingrédients et recettes, je calcule les contraintes sur la MN qui sont imposées par le fond diffus gamma. Je considère les données de FERMI (1ere année) et je les compare aux prédictions d'annihilation et désintégration de MN. Enfin, comme les annihilations de MN après recombinaison et pendant l'époque de la formation des structures déposent de l'énergie dans le milieu intergalactique primordial, j’enquête également sur les contraintes imposées par la profondeur optique observée de l'Univers. En ce qui concerne la construction de modèles, je présente deux modèles jouets de MN qui peuvent échapper aux contraintes actuelles de détection directe. Ils sont fondés sur l'hypothèse que les forces entre les deux secteurs pourraient ne pas être à courte portée
In this Ph. D. Thesis I have tried to summarize the Dark Matter (DM) phenomenology in ail aspects: Direct Detection, Indirect Detection and some aspects of mode! building. This is a very promising area as the profusion of ground and satellite-based measurements in recent years has rapidly advanced the field making it dynamic and timely. Concerning DM direct detection I review the main ingredients and recipes for Computing signals due to a WIMP-nucleus scattering I present the analytic treatment that allows us to derive the theoretical rate expected and, considering a standard choice in the features of the DM Halo and interaction cross section (point-like interaction), I report the current fits and constraints on DM properties. Concerning DM indirect detection, I provide the most advanced ingredients and recipes for Computing signals of TeV-scale DM annihilations and decays. Subsequently considering these ingredients and recipes, I compute the gamma ray constraints on DM properties that are imposed by the observed diffuse gamma rays. ] consider the data from FERMI first year observations and I compare them to the gamma rays fluxes predicted by DM annihilation and decays. Finally, as DM annihilations after recombination and during the epoch of structure formation deposit energy in the primordial intergalactic medium, I also investigate the constraints that are imposed by the observed optical depth of the Universe. Concerning model building, I present two DM toy mode 1s that can evade the current constraints on direct detection searches. They are based on the assumption that the forces between the two sectors might not be short range
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Baldi, Marco. "Interactions between Dark Energy and Dark Matter." Diss., lmu, 2009. http://nbn-resolving.de/urn:nbn:de:bvb:19-101617.

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Ciocia, Giuseppe. "Emerging dark matter from corpuscular dark energy." Master's thesis, Alma Mater Studiorum - Università di Bologna, 2021. http://amslaurea.unibo.it/23294/.

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In the last years, the standard model of cosmology has been corroborated by a wide number of astrophysical observations. Despite its undeniable success, nowadays there is little knowledge about the true nature of dark matter and dark energy. In this thesis we use a different approach to give an intriguing answer to these open problems, in the light of the corpuscular model of gravity. We give a general overview on the reasons behind the need for a corpuscular theory of the gravitational interaction. Then, we show that if the same picture is extended to cosmological spaces, dark energy naturally emerges as a quantum state of the gravitational dynamics, and it is described as a Bose-Einstein condensate of very soft and virtual gravitons without the necessity of introducing an exotic dark fluid. Besides, the cosmic condensate responds locally to the presence of baryonic matter, and the back-reaction manifests itself in the emergence of a dark force that mimics a dark matter behavior. In particular, at galactic scales the MOND formula for the acceleration is recovered. Then, a first attempt of estimating the back-reaction is proposed within the framework of Bootstrapped Newtonian gravity, that allows for an effective field description where Newtonian theory is “bootstrapped" introducing post-Newtonian corrections, providing a useful tool for calculations. Finally, we show that a logarithmic potential arises as a solution of the Bootstrapped field equation, in accordance with MOND prediction.
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Mondragon, Antonio Richard. "Lorentz-violating dark matter." [College Station, Tex. : Texas A&M University, 2007. http://hdl.handle.net/1969.1/ETD-TAMU-1672.

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D'Eramo, Francesco. "Hot and dark matter." Thesis, Massachusetts Institute of Technology, 2012. http://hdl.handle.net/1721.1/76977.

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Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 2012.
Cataloged from PDF version of thesis.
Includes bibliographical references (p. 253-273).
In this thesis, we build new Effective Field Theory tools to describe the propagation of energetic partons in hot and dense media, and we propose two new reactions for dark matter in the early universe. In the first part, we analyze the transverse momentum broadening in the absence of radiation of an energetic parton propagating through quark-gluon plasma via Soft Collinear Effective Theory (SCET). We show that the probability for picking up transverse momentum ki is given by the Fourier transform of the expectation value of two transversely separated light-like path-ordered Wilson lines. We evaluate the result for the strongly coupled plasma of N = 4 SYM theory by using gauge/gravity duality, and for the weakly coupled QCD plasma by using perturbation theory. In the second part, we introduce two new dark matter reactions, called "semi-annihilation" and "assimilation". The semi-annihilation reaction takes the schematic form [psi]i[psi]j -> [psi]k[psi], where [psi]i are stable dark matter particles and # is an unstable state. They lead to non-trivial dark matter dynamics in the early universe, and they might also take place today in the Milky Way, enriching the (semi-)annihilation final state spectrum observed in indirect detection experiments. The "assimilation" reaction efficiently destroy singlet dark matter particles, but dark matter number is stored in new quasi-stable heavy states which carry the baryon asymmetry. The subsequent annihilation and late-time decay of these heavy states yields (symmetric) dark matter as well as (asymmetric) standard model baryons.
by Francesco D'Eramo.
Ph.D.
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Mussie, Ezana. "Dark Matter, White Space." Thesis, Malmö universitet, Fakulteten för kultur och samhälle (KS), 2019. http://urn.kb.se/resolve?urn=urn:nbn:se:mau:diva-21571.

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This thesis addresses the ambiguous role of Malmö’s latest megaproject in the context of the city’s racializing urban development trajectory. The project is a public/private congress center, concert hall and hotel complex called Malmö Live. Malmö Live is problematized as the height of spectacle and challenge as it is expected to be the city’s most prominent cultural and social meeting place. The inquiry is directed to how its expectation of relevancy came about and utilizes a Foucauldian inspired genealogical methodology. The result stems from an investigation of the historical, present, local and global conditions that constitutes the expectancy of its relevancy. The investigation notes the divisiveness of tourism and how it affects ways of thinking and doing government on multiple scales, and in particular how it motivates the case in question. The result shows that there are affinities between tourism- during-colonialism and the contemporary tourism industry. Where the former was appropriated by colonialism and overtly racializing, the latter is allowed appropriacy by a currency ascribed to selected geographies and histories. By describing the becoming of this megaproject and the use of tourism knowledge and technology, the how-question about the expectation of Malmö Live’s relevancy leads to a genealogical reconstruction of Malmö Live as a wager on whiteness. The wager on whiteness hold no guarantees, but the power of it is the ability to be persuasive and believed, and the currency it holds for those who perform it. The thesis ends with a discussion on what is at stake with Malmö Live, i.e. Malmö’s whiteness.
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McEwen, Joseph Eugene McEwen. "The Hidden Universe: Dark Energy, Dark Matter, Baryons." The Ohio State University, 2016. http://rave.ohiolink.edu/etdc/view?acc_num=osu1471877488.

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Books on the topic "Dark matter"

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Perkins, Michael. Dark matter. London: Eros Plus, 1996.

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Cruise, Cameron. Dark Matter. Toronto, Ontario: MIRA, 2008.

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Newman, Randy. Dark matter. Place of publication not identified]: Nonesuch, 2017.

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Thomas, Sheree Renée. Dark Matter. New York: Grand Central Publishing, 2004.

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Zeh, Juli. Dark matter. London: Harvill Secker, 2010.

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Perkins, Michael. Dark matter. New York: Blue Moon, 1996.

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Reeves-Stevens, Garfield. Dark matter. New York: Bantam Books, 1991.

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Cruise, Cameron. Dark matter. Don Mills, Ont: Mira, 2008.

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Zeh, Juli. Dark matter. London: Harvill Secker, 2010.

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Reeves-Stevens, Garfield. Dark matter. New York: Doubleday, 1990.

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Book chapters on the topic "Dark matter"

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De Rújula, A. "Dark Matter." In The Challenging Questions, 23–31. Boston, MA: Springer US, 1990. http://dx.doi.org/10.1007/978-1-4615-3828-8_2.

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Pöttgen, Ruth. "Dark Matter." In Search for Dark Matter with ATLAS, 21–43. Cham: Springer International Publishing, 2016. http://dx.doi.org/10.1007/978-3-319-41045-6_3.

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Gramling, Johanna. "Dark Matter." In Search for Dark Matter with the ATLAS Detector, 21–39. Cham: Springer International Publishing, 2018. http://dx.doi.org/10.1007/978-3-319-95016-7_3.

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Mohanty, Subhendra. "Dark Matter." In 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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Rhee, George. "Dark Matter." In Astronomers' Universe, 89–116. New York, NY: Springer New York, 2013. http://dx.doi.org/10.1007/978-1-4614-7813-3_4.

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Sancisi, R., and T. S. van Albada. "Dark Matter." In Observational Cosmology, 699–712. Dordrecht: Springer Netherlands, 1987. http://dx.doi.org/10.1007/978-94-009-3853-3_82.

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Bari, Pasquale Di. "Dark matter." In Cosmology and the Early Universe, 211–35. Boca Raton : CRC Press, [2018] | Series: Series in astronomy and astrophysics: CRC Press, 2018. http://dx.doi.org/10.1201/9781138496903-17.

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Sigl, Günter. "Dark Matter." In 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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Silk, Joseph. "Dark Matter." In NATO ASI Series, 237–50. Boston, MA: Springer US, 1997. http://dx.doi.org/10.1007/978-1-4899-0242-9_13.

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Bambi, Cosimo, and Alexandre D. Dolgov. "Dark Matter." In 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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Conference papers on the topic "Dark matter"

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Postman, Marc. "Using galaxy clusters to trace the large scale velocity field." In Dark matter. AIP, 1995. http://dx.doi.org/10.1063/1.48360.

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Broadhurst, Tom. "Mass distributions of clusters from gravitational magnification." In Dark matter. AIP, 1995. http://dx.doi.org/10.1063/1.48351.

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Khan, Irshadullah. "The nature of dark matter and galactic rotation curves." In Dark matter. AIP, 1995. http://dx.doi.org/10.1063/1.48321.

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Bertola, Francesco, and Alessandro Pizzella. "Dark matter in elliptical galaxies." In Dark matter. AIP, 1995. http://dx.doi.org/10.1063/1.48323.

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Kazanas, Demosthenes. "Alternatives to dark matter." In Dark matter. AIP, 1995. http://dx.doi.org/10.1063/1.48382.

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Mannheim, Philip D. "Microlensing, Newton-Einstein gravity, and conformal gravity." In Dark matter. AIP, 1995. http://dx.doi.org/10.1063/1.48383.

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Buote, David A., and Claude R. Canizares. "X-ray constraints on the intrinsic shape of the lenticular galaxy NGC 1332." In Dark matter. AIP, 1995. http://dx.doi.org/10.1063/1.48312.

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Pfenniger, Daniel, and Françoise Combes. "Cold molecular gas as dark matter candidate in galaxies and clusters." In Dark matter. AIP, 1995. http://dx.doi.org/10.1063/1.48384.

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Canizares, Claude R., and David A. Buote. "Constraints on dark matter in clusters & galaxies from the shapes of X-ray images." In Dark matter. AIP, 1995. http://dx.doi.org/10.1063/1.48313.

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Wilczek, Frank. "From the standard model to dark matter." In Dark matter. AIP, 1995. http://dx.doi.org/10.1063/1.48314.

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Reports on the topic "Dark matter"

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Baltz, E. Dark Matter Candidates. Office of Scientific and Technical Information (OSTI), December 2004. http://dx.doi.org/10.2172/839811.

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Essig, Rouven. Searching for Dark Matter and Dark Sectors. Office of Scientific and Technical Information (OSTI), April 2020. http://dx.doi.org/10.2172/1664761.

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Sikivie, P. Dark matter axions `96. Office of Scientific and Technical Information (OSTI), December 1996. http://dx.doi.org/10.2172/446290.

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Wai, Lawrence L. GLAST DARK MATTER SEARCH. Office of Scientific and Technical Information (OSTI), November 2002. http://dx.doi.org/10.2172/808683.

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Cohen, Timothy, John Kearney, Aaron Pierce, and David Tucker-Smith. Singlet-Doublet Dark Matter. Office of Scientific and Technical Information (OSTI), February 2012. http://dx.doi.org/10.2172/1035103.

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Rielage, Keith. Introduction to Dark Matter. Office of Scientific and Technical Information (OSTI), March 2024. http://dx.doi.org/10.2172/2323515.

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Brown, Benjamin. Special Gravity #1 - Dark Energy and Dark Matter. ResearchHub Technologies, Inc., September 2023. http://dx.doi.org/10.55277/researchhub.idocddli.

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Scherrer, Robert. Theoretical Studies in Dark Energy and Dark Matter. Office of Scientific and Technical Information (OSTI), May 2023. http://dx.doi.org/10.2172/1972343.

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Moskalenko, Igor V., and L. Wai. Dark Matter Burners: Preliminary Estimate. Office of Scientific and Technical Information (OSTI), September 2006. http://dx.doi.org/10.2172/907961.

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Wai, Lawrence. Dark Matter Searches With GLAST. US: Stanford Linear Accelerator Center (SLAC), February 2007. http://dx.doi.org/10.2172/899208.

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