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Gotowa bibliografia na temat „Supersymmetry - Dark Matter”

Autor: Grafiati

Data publikacji: 7 września 2023

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Artykuły w czasopismach na temat "Supersymmetry - Dark Matter"

Heinemeyer, Sven, i Carlos Muñoz. "Dark Matter in Supersymmetry". Universe 8, nr 8 (18.08.2022): 427. http://dx.doi.org/10.3390/universe8080427.

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Supersymmetry is a well-motivated theory for physics beyond the Standard Model. In particular, supersymmetric models can naturally possess dark matter candidates that can give rise to the measured dark matter content of the universe. We review several models that have been analyzed with regard to dark matter by groups based in Spain in recent years. These models include, in particular, the Minimal Supersymmetric Standard Model (MSSM) and the ‘μ from ν’ Supersymmetric Standard Model (μνSSM) in various versions.

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Behbahani, Siavosh R., Martin Jankowiak, Tomas Rube i Jay G. Wacker. "Nearly Supersymmetric Dark Atoms". Advances in High Energy Physics 2011 (2011): 1–34. http://dx.doi.org/10.1155/2011/709492.

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Theories of dark matter that support bound states are an intriguing possibility for the identity of the missing mass of the Universe. This article proposes a class of models of supersymmetric composite dark matter where the interactions with the Standard Model communicate supersymmetry breaking to the dark sector. In these models, supersymmetry breaking can be treated as a perturbation on the spectrum of bound states. Using a general formalism, the spectrum with leading supersymmetry effects is computed without specifying the details of the binding dynamics. The interactions of the composite states with the Standard Model are computed, and several benchmark models are described. General features of nonrelativistic supersymmetric bound states are emphasized.

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GOGOLADZE, ILIA, RIZWAN KHALID, SHABBAR RAZA i QAISAR SHAFI. "NEUTRALINO DARK MATTER IN FLIPPED SU(5)". Modern Physics Letters A 25, nr 40 (28.12.2010): 3371–79. http://dx.doi.org/10.1142/s0217732310034602.

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We investigate neutralino dark matter in supersymmetric flipped SU(5), focusing on candidates with masses of order 30–150 GeV and spin-independent cross-sections that are consistent with the most recent CDMS II results. We assume gravity mediated supersymmetry breaking and restrict the magnitude of the soft supersymmetry breaking mass parameters to 1 TeV or less. With non-universal soft gaugino and Higgs masses, and taking flipped SU(5) into account, we identify allowed regions of the parameter space and highlight some benchmark solutions including Higgs and sparticle spectroscopy.

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Olive, Keith A. "Supersymmetric versus SO(10) models of dark matter". International Journal of Modern Physics A 32, nr 13 (5.05.2017): 1730010. http://dx.doi.org/10.1142/s0217751x17300101.

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After the results of Run I, can we still “guarantee” the discovery of supersymmetry at the LHC? It is shown that viable dark matter candidates in CMSSM-like models tend to lie in strips (coannihilation, funnel, focus point) in parameter space. The role of grand unification in constructing supersymmetric models is discussed and it is argued that nonsupersymmetric GUTs such as SO(10) may provide alternative solutions to many of the standard problems addressed by supersymmetry.

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Capolupo, Antonio. "Quantum Vacuum, Dark Matter, Dark Energy, and Spontaneous Supersymmetry Breaking". Advances in High Energy Physics 2018 (10.04.2018): 1–7. http://dx.doi.org/10.1155/2018/9840351.

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We study the behavior of the vacuum condensates characterizing many physical phenomena. We show that condensates due to thermal states, to fields in curved space, and to neutrino mixing, may represent new components of the dark matter, whereas the condensate due to axion-photon mixing can contribute to the dark energy. Moreover, by considering a supersymmetric framework, we show that the nonzero energy of vacuum condensates may induce a spontaneous supersymmetry breaking.

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Roszkowski, Leszek. "Supersymmetry and dark matter". Nuclear Physics B - Proceedings Supplements 124 (lipiec 2003): 30–37. http://dx.doi.org/10.1016/s0920-5632(03)02074-7.

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Addazi, Andrea, i Maxim Yu Khlopov. "Dark matter from Starobinsky supergravity". Modern Physics Letters A 32, nr 15 (11.04.2017): 1740002. http://dx.doi.org/10.1142/s0217732317400028.

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We review our recent results on dark matter from Starobinsky supergravity. In this context, a natural candidate for cold dark matter is the gravitino. On the other hand, assuming the supersymmetry broken at scales much higher than the electroweak scale, gravitinos are superheavy particles. In this case, they may be non-thermally produced during inflation, in turn originated by the scalaron field with Starobinsky’s potential. Assuming gravitinos as Lightest Supersymmetric Particles (LSSP), the non-thermal production naturally accounts for the right amount of cold dark matter. Metastability of the gravitino LSSP leads to observable effects of their decay, putting constraints on the corresponding Unstable or Decaying Dark Matters scenarios. In this model, the gravitino mass is controlled by the inflaton field and it runs with it. This implies that a continuous spectrum of superheavy gravitinos is produced during the slow-roll epoch. Implications in phenomenology, model building in Grand Unified Theory (GUT) scenarios, intersecting D-brane models and instantons in string theories are discussed.

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LAHANAS, A. B., N. E. MAVROMATOS i D. V. NANOPOULOS. "WMAPing THE UNIVERSE: SUPERSYMMETRY, DARK MATTER, DARK ENERGY, PROTON DECAY AND COLLIDER PHYSICS". International Journal of Modern Physics D 12, nr 09 (październik 2003): 1529–91. http://dx.doi.org/10.1142/s0218271803004286.

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In this review we critically discuss constraints on minimal supersymmetric models of particle physics as implied by the recent astrophysical observations of WMAP satellite experiment. Although the prospects of detecting supersymmetry increase dramatically, at least within the context of the minimal models, and 90% of the available parameter space can safely be reached by the sensitivity of future colliders, such as Tevatron, LHC and linear colliders, nevertheless we pay particular emphasis on discussing regions of the appropriate phase diagrams, which — if realized in nature — would imply that detection of supersymmetry, at least in the context of minimal models, could be out of colliders reach. We also discuss the importance of a precise determination of the radiative corrections to the muon anomalous magnetic moment, gμ-2, both theoretically and experimentally, which could lead to elimination of such "out of reach" regions in case of a confirmed discrepancy of gμ-2 from the standard model value. Finally, we briefly commend upon recent evidence, supported by observations, on a dark energy component of the Universe, of as yet unknown origin, covering 73% of its energy content. To be specific, we discuss how supergravity quintessence (relaxation) models can be made consistent with recent observations, which may lead to phenomenologically correct constrained supersymmetric models, accounting properly for this dark energy component. We also outline their unresolved problems.

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Shaposhnikov, Mikhail. "Superheavy dark matter and supersymmetry". New Astronomy Reviews 49, nr 2-6 (maj 2005): 175–79. http://dx.doi.org/10.1016/j.newar.2005.03.001.

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Lopez, Jorge L., Kajia Yuan i D. V. Nanopoulos. "Supersymmetry breaking and dark matter". Physics Letters B 267, nr 2 (wrzesień 1991): 219–26. http://dx.doi.org/10.1016/0370-2693(91)91251-p.

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Rozprawy doktorskie na temat "Supersymmetry - Dark Matter"

Han, Tao, Felix Kling, Shufang Su i Yongcheng Wu. "Unblinding the dark matter blind spots". SPRINGER, 2017. http://hdl.handle.net/10150/623247.

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The dark matter (DM) blind spots in the Minimal Supersymmetric Standard Model (MSSM) refer to the parameter regions where the couplings of the DM particles to the Z-boson or the Higgs boson are almost zero, leading to vanishingly small signals for the DM direct detections. In this paper, we carry out comprehensive analyses for the DM searches under the blind-spot scenarios in MSSM. Guided by the requirement of acceptable DM relic abundance, we explore the complementary coverage for the theory parameters at the LHC, the projection for the future underground DM direct searches, and the indirect searches from the relic DM annihilation into photons and neutrinos. We find that (i) the spin-independent (SI) blind spots may be rescued by the spin-dependent (SD) direct detection in the future underground experiments, and possibly by the indirect DM detections from IceCube and SuperK neutrino experiments; (H) the detection of gamma rays from Fermi-LAT may not reach the desirable sensitivity for searching for the DM blind spot regions; (Hi) the SUSY searches at the LHC will substantially extend the discovery region for the blind-spot parameters. The dark matter blind spots thus may be unblinded with the collective efforts in future DM searches.

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Silverwood, Hamish George Miles. "Supersymmetric Dark Matter in IceCube". Thesis, University of Canterbury. Physics and Astronomy, 2012. http://hdl.handle.net/10092/6927.

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The Minimally Supersymmetric Standard Model (MSSM) provides us with a WIMP dark matter candidate particle, the neutralino. Neutralinos from the dark matter halo can potentially become captured by the sun and concentrated in the core, where they can undergo self-annihilation and so produce a distinct neutrino signal. The IceCube Neutrino Observatory has the potential to detect this neutrino signal and thus give indirect evidence of the presence and properties of neutralino dark matter. Although the full, unconstrained MSSM has 105 parameters this can be reduced to 25 parameters by the application of physically motivated assumptions. Scans of this MSSM-25 parameter space are conducted using the DarkSUSY software package and an adaptive scanning technique based on the Monte-Carlo VEGAS algorithm. The IceCube exclusion confidence level is then calculated for a set of points produced by these scans. Results indicate that the detection capability of IceCube exceeds that of current direct detection methods in certain regions of the parameter space. The use of a 25 dimensional parameter space reveals that there are new regions of observables with high exclusion confidence levels compared to earlier simulations performed with a seven dimensional parameter space.

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Raj, Nirmal. "Dark Matter and Supersymmetry in the LHC Era". Thesis, University of Oregon, 2015. http://hdl.handle.net/1794/19253.

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We report investigations of physical possibilities beyond the Standard Model, performed in the years between Runs I and II of the Large Hadron Collider (LHC). First, we explore the feasibility of using a hadron collider to unmask hidden sectors by means of a novel signal, the ``monocline". Dilepton production provides the cleanest channel to anticipate a monocline. A compelling sector to seek is dark matter with scalar messengers coupling it to standard fermions. We present current bounds from dilepton spectrum measurements at the LHC and make predictions for sensitivities at Run II of the LHC as well as at a future 100 TeV collider. Second, we corner the space of parameters of supersymmetric frameworks with an appreciable Yukawa coupling between the Higgs fields and a gauge singlet, the so-called Fat Higgs and $\lambda$-SUSY models, in the context of the discovery of the 125 GeV Higgs particle. These models are motivated by their alleviation of the electroweak fine-tuning that supersymmetry breaking entails, via raising the tree-level quartic coupling Higgs boson. Heavy Higgs scalars that couple strongly to the standard Higgs boson induce large radiative corrections to the Higgs quartic coupling, which is crucial to phenomenology; in particular, a very large ratio of the Higgs VEVs ($\tan \beta$), that was previously presumed unfavorable in these models, becomes viable and can be probed by future experiments. In such regions, the most stringent limits come from dark matter constraints on the lightest neutralino. Finally, we place limits on colored scalar production at the LHC in supersymmetric models where gauginos acquire both Dirac and Majorana masses, that we call ``mixed gauginos". While it was known that purely Dirac gluinos were less constrained by LHC searches than their purely Majorana counterparts, we find that the constraints further weaken or strengthen depending on which of the ``mixed" colored fermions acquires a Majorana mass. Also explored are the effects on squark production of turning on Majorana masses for electroweak gauginos. This dissertation consists of previously published and unpublished co-authored material.

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Schelke, Mia. "Supersymmetric Dark Matter : aspects of sfermion coannihilations". Doctoral thesis, Stockholm : Fysikum, Univ, 2004. http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-192.

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West, Stephen Mathew. "Neutrino masses, leptogenesis and dark matter from supersymmetry breaking". Thesis, University of Oxford, 2005. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.491611.

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In this thesis, we analyse a class of supersymmetric models first introduced by ArkaniHamed et al and Borzumati et al. in which the light neutrino masses result from higherdimensional supersymmetry-breaking terms in the M88M super- and Kahler-potentials. The mechanism is closely related to the Giudice-Masiero mechanism for the M88M p, parameter, and leads to TeV-scale right-handed neutrino and sneutrino states. The dominant contribution to the light neutrino (Majorana) mass matrix is a one-loop term with a sub-dominant tree-level 'see-saw' contribution which may lead to interesting perturbations of the leading flavour structure, possibly generating the small ratio !:lm;olarl!:lm~tm dynamically. Using this mechanism it is also possible to construct a natural model of TeV-scale resonant leptogenesis. The model leads to large cosmological lepton asymmetries via the resonant behaviour of the one-loop self-energy contribution to the right-handed neutrino (Ni ) decay. This model addresses the primary problems of previous phenomenological studies of low-energy leptogenesis: a rational for TeV-scale right-handed neutrinos with small Yukawa couplings so that the out-of equilibrium condition for Ni decay is satisfied; the origin of the tiny, but non-zero mass splitting required between at least t,vo Ni masses; and the necessary non-trivial breaking of flavour symmetries in the right-handed neutrino sector. Following this, a weakly broken gauged 80(3) flavour symmetry is used to produce. two highly-degenerate right-handed neutrinos. It is shown that this 80(3) flavour symmetry is compatible with all fermion masses and mixings if it is supplemented with a further 8U(3) flavour symmetry. This mechanism is then embedded into the model of neutrino masses and leptogenesis described above. Lastly, we investigate why the inferred values of the cosmological baryon and dark matter densities are so strikingly similar. We consider models of dark matter possessing a particle-antiparticle asymmetry where this asymmetry determines both the baryon asymmetry and strongly effects the dark matter density, thus naturally linking Ob and 0dm. We show that sneutrinos can play the role of such dark matter.

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McCullough, Matthew Philip. "Topics in BSM physics : supersymmetry, dark matter and baryogenesis". Thesis, University of Oxford, 2011. http://ora.ox.ac.uk/objects/uuid:f2a6c703-8b95-4345-9477-4afeea355a8e.

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Under the umbrella of Theoretical Physics, progress in ‘Beyond the Standard Model’ (BSM) physics proceeds broadly along two main avenues of investigation. The first is concerned with constructing theories that attempt to explain observations, or address theoretical problems, which cannot be explained within the tremendously successful Standard Model (SM) of particle physics. The second involves looking for new ways to observe or test BSM physics, and such tests are usually developed with current experimental hints, or attractive theoretical models, in mind. This thesis contains material which falls under both approaches. Part I is concerned with Supersymmetry (SUSY). We review the basics of SUSY, and the current state of this field, and then present a novel model for SUSY at the TeV scale. This model has a Higgs sector similar to the SM and possesses a continuous U(1)_R symmetry, dramatically suppressing contributions to flavour-changing neutral currents, which can be problematic in SUSY models. After this we demonstrate that if more than one SUSY-breaking sector is present then this could lead to a rich spectrum of states with mass roughly twice the gravitino mass. In particular, if SUSY-breaking in a hidden sector arises dynamically then multiple ‘Goldstini’ and ‘Modulini’ states can arise, which couple to visible sector fields via the ‘Goldstino Portal’. We also demonstrate a new phenomenon which can occur in the context of multiple hidden sectors. If one sector breaks SUSY then this can ‘stimulate’ other sectors into also breaking SUSY, even if they are incapable of doing so on their own. Part II focusses on the matter in our Universe. We review our current understand- ing of how the visible matter in our Universe came into existence, and our current understanding of the nature of dark matter (DM). Following this we describe how DM could potentially be indirectly observed through its effects on cold white dwarf stars. Alternatively, if DM were detected by independent means, then observed cold white dwarfs could be used to place limits on the DM density in globular clusters, giving clues as to how these clusters of stars formed. We then present a new model for the co-generation of both the visible and dark matter in our Universe. This proceeds by generating a particle anti-particle asymmetry in the dark sector, which is then shared with the visible sector. This model predicts the existence of a light, m ≲ 5 eV, scalar particle which derivatively couples to DM, and provides a final state for the symmetric DM component to annihilate away into. Work completed during the period of this D.Phil is contained in [1–8], however only material in [3–6, 8] is presented in this thesis.

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Macias, Ramirez Oscar. "Astrophysical Constraints on Dark Matter". Thesis, University of Canterbury. Department of Physics and Astronomy, 2014. http://hdl.handle.net/10092/9857.

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Well motivated theoretical models predict the annihilation of dark matter (DM) into standard model particles, a phenomenon which could be a significant source of photons in the gamma-ray sky. With its unprecedented sensitivity and its broad energy range (20 MeV to more than 300 GeV) the main instrument on board the Fermi satellite, the Large Area Telescope (LAT), might be able to detect an indirect signature of DM annihilations. In this work we revisit several interesting claims of extended dark matter emission made from analyses of Fermi-LAT data: First, based on three years of Fermi Large Area Telescope (LAT) gamma-ray data of the Virgo cluster, evidence for an extended emission associated with dark matter pair annihilation in the bb̄ channel has been reported by Han et al. (arxiv:1201.1003). After an in depth spatial and temporal analysis, we argue that the tentative evidence for a gamma-ray excess from the Virgo cluster is mainly due to the appearance of a population of previously unresolved gamma-ray point sources in the region of interest. These point sources are not part of the LAT second source catalogue (2FGL), but are found to be above the standard detection significance threshold when three or more years of LAT data is included. Second, we confirm the detection of a spatially extended excess of 2-5 GeV gamma rays from the Galactic Center (GC), consistent with the emission expected from annihilating dark matter or an unresolved population of about 10³ milisecond pulsars. However, there are significant uncertainties in the diffuse galactic background at the GC. We have performed a revaluation of these two models for the extended gamma ray source at the GC by accounting for the systematic uncertainties of the Galactic diffuse emission model. We also marginalize over point source and diffuse background parameters in the region of interest. We show that the excess emission is significantly more extended than a point source. We find that the DM (or pulsars population) signal is larger than the systematic errors and therefore proceed to determine the sectors of parameter space that provide an acceptable fit to the data. We found that a population of order a 10³ MSPs with parameters consistent with the average spectral shape of Fermi-LAT measured MSPs was able to fit the GC excess emission. For DM, we found that a pure τ⁺τ⁻ annihilation channel is not a good fit to the data. But a mixture of τ⁻τ⁻ and bb̄ with a (σν) of order the thermal relic value and a DM mass of around 20 to 60 GeV provides an adequate fit. We also consider the possibility that the GeV excess is due to nonthermal bremsstrahlung produced by a population of electrons interacting with neutral gas in molecular clouds. The millisecond pulsars and dark matter alternatives have spatial templates well fitted by the square of a generalized Navarro-Frenk-White (NFW) profile with inner slope γ = 1.2. We model the third option with a 20-cm continuum emission Galactic Ridge template. A template based on the HESS residuals is shown to give similar results. The gamma-ray excess is found to be best fit by a combination of the generalized NFW squared template and a Galactic Ridge template. We also find the spectra of each template is not significantly affected in the combined fit and is consistent with previous single template fits. That is, the generalized NFW squared spectrum can be fit by either of order 10³ unresolved MSPs or DM with mass around 30 GeV, a thermal cross section, and mainly annihilating to bb̄ quarks. While the Galactic Ridge continues to have a spectrum consistent with a population of nonthermal electrons whose spectrum also provides a good fit to synchrotron emission measurements. We also show that the current DM fit may be hard to test, even with 10 years of Fermi-LAT data, especially if there is a mixture of DM and MSPs contributing to the signal, in which case the implied DM cross section will be suppressed.

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McCabe, Christopher. "Aspects of dark matter phenomenology". Thesis, University of Oxford, 2011. http://ora.ox.ac.uk/objects/uuid:74ec0d09-40d6-481d-b2ec-d0e9d41d5c1d.

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Identifying the relic particles that constitute the cold dark matter in our Universe is an outstanding problem in astro-particle physics. Direct detection experiments are among the most promising methods of detecting particle dark matter through non-gravitational interactions. In this thesis, the usual assumptions made when calculating the event rate at direct detection experiments are examined. Varying astrophysical parameters and the dark matter velocity distribution leads to significant changes in acceptance regions and exclusion curves for scenarios in which the tail of the velocity distribution is sampled; this includes 'light dark matter' (mass less than 10 GeV) and 'inelastic dark matter'. The DAMA and CoGeNT collaborations both report an annual modulation in their event rate that they attribute to dark matter. Two analyses of these experiments are performed. In the first, it is shown that these experiments can be compatible with each other and with the constraints from other direct detection experiments. This requires some isospin violation in the couplings of dark matter to protons and neutrons and a small inelastic splitting to boost the modulation fraction. The second analysis provides a comparison of the modulation signals free from all astrophysical parameters, under the assumption that dark matter scatters elastically. Again it is found that some isospin violation and a boosted modulation fraction is required in order that DAMA and CoGeNT are consistent with all experiments. A boosted modulation fraction may arise from a velocity distribution different from the Maxwell-Boltzmann distribution, which is usually assumed. Finally, a supersymmetric theory in which the dark matter candidate is a mixture of left- and right-handed sneutrino is considered. This theory has many novel signatures at colliders, indirect detection and direct detection experiments.

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Gustafsson, Michael. "Light from Dark Matter : Hidden Dimensions, Supersymmetry, and Inert Higgs". Doctoral thesis, Stockholm : Department of Physics, Stockholm university, 2008. http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-7345.

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Dumont, Béranger. "Higgs, supersymmetry and dark matter after Run I of the LHC". Thesis, Grenoble, 2014. http://www.theses.fr/2014GRENY025/document.

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Deux problèmes majeurs requièrent une extension du Modèle Standard (MS) : le problème de hiérarchie dans le secteur de Higgs, et la matière noire de notre Univers. La découverte d'un boson de Higgs avec une masse d'environ 125 GeV est clairement l'événement majeur en provenance du Large Hadron Collider (LHC) du CERN. Cela représente le triomphe définitif du MS, mais cela met également en lumière le problème de hiérarchie et ouvre de nouvelles voies pour sonder la nouvelle physique. Les différentes mesures effectuées pendant le run I du LHC contraignent les couplages du Higgs aux particules du MS ainsi que les désintégrations invisibles et non-détectées. Dans cette thèse, l'impact des résultats sur le boson de Higgs au LHC est étudié dans le cadre de différents modèles de nouvelle physique, en prenant soigneusement en compte les incertitudes et leurs corrélations. Des modifications génériques à la force des couplages du Higgs (pouvant provenir de secteurs de Higgs étendus ou d'opérateurs de dimension supérieure) sont étudiées. De plus, des modèles de nouvelle physique spécifiques sont testés, notamment, mais pas seulement, le Modèle Standard Supersymétrique Minimal phénoménologique.Alors qu'un boson de Higgs a été trouvé, il n'y a toutefois nulle trace de physique au-delà du MS au run I du LHC en dépit du grand nombre de recherches effectuées par les collaborations ATLAS et CMS. Les conséquences des résultats négatifs obtenus lors de ces recherches constituent un autre volet important de cette thèse. Tout d'abord, des modèles supersymétriques avec un candidat à la matière noire sont étudiés à la lumière des résultats négatifs dans les recherches de supersymétrie au LHC, en utilisant une approche basée sur les "modèles simplifiés". Ensuite, des outils pour contraindre un modèle de nouvelle physique quelconque à partir des résultats du LHC et d'événements simulés sont présentés. De plus, au cours de cette thèse, les critères de sélection de plusieurs analyses au-delà du MS ont été réimplémentés dans le cadre de MadAnalysis 5 et ont été intégrés à une base de données publique
Two major problems call for an extension of the Standard Model (SM): the hierarchy problem in the Higgs sector and the dark matter in the Universe. The discovery of a Higgs boson with mass of about 125 GeV was clearly the most significant piece of news from CERN's Large Hadron Collider (LHC). In addition to representing the ultimate triumph of the SM, it shed new light on the hierarchy problem and opened up new ways of probing new physics. The various measurements performed at Run I of the LHC constrain the Higgs couplings to SM particles as well as invisible and undetected decays. In this thesis, the impact of the LHC Higgs results on various new physics scenarios is assessed, carefully taking into account uncertainties and correlations between them. Generic modifications of the Higgs coupling strengths, possibly arising from extended Higgs sectors or higher-dimensional operators, are considered. Furthermore, specific new physics models are tested. This includes, in particular, the phenomenological Minimal Supersymmetric Standard Model.While a Higgs boson has been found, no sign of beyond the SM physics was observed at Run I of the LHC in spite of the large number of searches performed by the ATLAS and CMS collaborations. The implications of the negative results obtained in these searches constitute another important part of this thesis. First, supersymmetric models with a dark matter candidate are investigated in light of the negative searches for supersymmetry at the LHC using a so-called "simplified model" approach. Second, tools using simulated events to constrain any new physics scenario from the LHC results are presented. Moreover, during this thesis the selection criteria of several beyond the SM analyses have been reimplemented in the MadAnalysis 5 framework and made available in a public database

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Książki na temat "Supersymmetry - Dark Matter"

Dumont, Béranger. Higgs, Supersymmetry and Dark Matter After Run I of the LHC. Cham: Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-44956-2.

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1939-, Pran Nath, Alverson George Oscar 1951- i Nelson Brent, red. SUSY09: The 17th International Conference on Supersymmetry and the Unification of Fundamental Interactions, Boston, Massachusetts, 5-10 June 2009. Melville, N.Y: American Institute of Physics, 2009.

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

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Köhler, Nicolas Maximilian. Searches for the Supersymmetric Partner of the Top Quark, Dark Matter and Dark Energy at the ATLAS Experiment. Cham: Springer International Publishing, 2019. http://dx.doi.org/10.1007/978-3-030-25988-4.

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Basak, Tanushree. Approach to Dark Matter Modelling. Morgan & Claypool Publishers, 2018.

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Dumont, Béranger. Higgs, Supersymmetry and Dark Matter After Run I of the LHC. Springer, 2016.

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Dumont, Béranger. Higgs, Supersymmetry and Dark Matter After Run I of the LHC. Springer, 2018.

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Köhler, Nicolas Maximilian. Searches for the Supersymmetric Partner of the Top Quark, Dark Matter and Dark Energy at the ATLAS Experiment. Springer, 2019.

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Köhler, Nicolas Maximilian. Searches for the Supersymmetric Partner of the Top Quark, Dark Matter and Dark Energy at the ATLAS Experiment. Springer International Publishing AG, 2020.

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Części książek na temat "Supersymmetry - Dark Matter"

Arnowitt, R., i B. Dutta. "Supersymmetry and Dark Matter". W Dark Matter in Astro- and Particle Physics, 175–88. Berlin, Heidelberg: Springer Berlin Heidelberg, 2002. http://dx.doi.org/10.1007/978-3-642-55739-2_17.

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Gramling, Johanna. "Supersymmetry". W Search for Dark Matter with the ATLAS Detector, 41–50. Cham: Springer International Publishing, 2018. http://dx.doi.org/10.1007/978-3-319-95016-7_4.

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Catena, Riccardo, i Laura Covi. "SUSY dark matter(s)". W Supersymmetry After the Higgs Discovery, 121–36. Berlin, Heidelberg: Springer Berlin Heidelberg, 2014. http://dx.doi.org/10.1007/978-3-662-44172-5_7.

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Bianchi, Massimo, Roland Allen i Antonio Mondragon. "Dark Matter, Supersymmetry and Supergravity Models". W Concise Encyclopedia of Supersymmetry, 120–21. Dordrecht: Springer Netherlands, 2004. http://dx.doi.org/10.1007/1-4020-4522-0_148.

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Kusenko, Alexander. "Supersymmetry, Q-Balls, and Dark Matter". W Sources and Detection of Dark Matter and Dark Energy in the Universe, 248–55. Berlin, Heidelberg: Springer Berlin Heidelberg, 2001. http://dx.doi.org/10.1007/978-3-662-04587-9_26.

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Covi, Laura. "Models of Inflation, Supersymmetry Breaking and Observational Constraints". W Dark Matter in Astro- and Particle Physics, 163–75. Berlin, Heidelberg: Springer Berlin Heidelberg, 2001. http://dx.doi.org/10.1007/978-3-642-56643-1_18.

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Chattopadhyay, Utpal, Achille Corsetti i Pran Nath. "Status of Supersymmetry in the Light of Recent Experiments". W Dark Matter in Astro- and Particle Physics, 202–16. Berlin, Heidelberg: Springer Berlin Heidelberg, 2002. http://dx.doi.org/10.1007/978-3-642-55739-2_19.

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Baer, Howard. "Radiative Natural Supersymmetry with Mixed Axion/Higgsino Cold Dark Matter". W Springer Proceedings in Physics, 3–15. Dordrecht: Springer Netherlands, 2013. http://dx.doi.org/10.1007/978-94-007-7241-0_1.

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Lichtenberg, D. B. "Hadron Supersymmetry and Relations between Meson and Baryon Masses". W Neutrino Mass, Dark Matter, Gravitational Waves, Monopole Condensation, and Light Cone Quantization, 319–22. Boston, MA: Springer US, 1996. http://dx.doi.org/10.1007/978-1-4899-1564-1_29.

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Dumont, Béranger. "Introduction". W Higgs, Supersymmetry and Dark Matter After Run I of the LHC, 1–27. Cham: Springer International Publishing, 2016. http://dx.doi.org/10.1007/978-3-319-44956-2_1.

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Streszczenia konferencji na temat "Supersymmetry - Dark Matter"

ROSZKOWSKI, LESZEK. "DARK MATTER AND SUPERSYMMETRY". W Proceedings of the 7th International Heidelberg Conference on Dark 2009. WORLD SCIENTIFIC, 2009. http://dx.doi.org/10.1142/9789814293792_0005.

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SCOPEL, S. "DARK MATTER AND SUPERSYMMETRY". W Proceedings of the International Conference. WORLD SCIENTIFIC, 2004. http://dx.doi.org/10.1142/9789812702999_0032.

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Balazs, Csaba, Peter Athron, Benjamin Farmer i Doyoun Kim. "Naturalness, supersymmetry and dark matter". W 11th International Workshop Dark Side of the Universe 2015. Trieste, Italy: Sissa Medialab, 2016. http://dx.doi.org/10.22323/1.268.0028.

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de Boer, Wim, Pyungwon Ko i Deog Ki Hong. "Indirect Dark Matter Signals". W SUPERSYMMETRY AND THE UNIFICATION OF FUNDAMENTAL INTERACTIONS. AIP, 2008. http://dx.doi.org/10.1063/1.3051890.

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Shin, Seodong, Pyungwon Ko i Deog Ki Hong. "Singlet fermionic dark matter". W SUPERSYMMETRY AND THE UNIFICATION OF FUNDAMENTAL INTERACTIONS. AIP, 2008. http://dx.doi.org/10.1063/1.3052027.

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Fayet, Pierre. "Supersymmetry, dark matter and new particles". W FRONTIERS OF FUNDAMENTAL PHYSICS: The Eleventh International Symposium. AIP, 2012. http://dx.doi.org/10.1063/1.4727989.

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Provenza, A., M. Quiros i P. Ullio. "Dark Matter in split extended supersymmetry". W SUSY06: THE 14TH INTERNATIONAL CONFERENCE ON SUPERSYMMETRY AND THE UNIFICATION OF FUNDAMENTAL INTERACTIONS. AIP, 2007. http://dx.doi.org/10.1063/1.2735252.

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Fayet, Pierre, Jean-Michel Alimi i André Fuözfa. "SUPERSYMMETRY, DARK MATTER AND NEW PARTICLES". W INVISIBLE UNIVERSE: Proceedings of the Conference. AIP, 2010. http://dx.doi.org/10.1063/1.3462718.

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HOOPER, DAN. "STUDYING SUPERSYMMETRY WITH DARK MATTER EXPERIMENTS". W Proceedings of the Sixth International Workshop. WORLD SCIENTIFIC, 2007. http://dx.doi.org/10.1142/9789812770288_0004.

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Tata, Xerxes, George Alverson, Pran Nath i Brent Nelson. "Supersymmetry, Dark Matter and the LHC". W SUSY09: 7th International Conference on Supersymmetry and the Unification of Fundamental Interactions. AIP, 2010. http://dx.doi.org/10.1063/1.3327553.

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Raporty organizacyjne na temat "Supersymmetry - Dark Matter"

Kitano, Ryuichiro, i Yasunori Nomura. Supersymmetry with Small mu: Connections between Naturalness, Dark Matter, and (Possibly) Flavor. Office of Scientific and Technical Information (OSTI), czerwiec 2006. http://dx.doi.org/10.2172/885275.

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Gondolo, P. DarkSUSY: Computing Supersymmetric Dark Matter Properties Numerically. Office of Scientific and Technical Information (OSTI), lipiec 2004. http://dx.doi.org/10.2172/827305.

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Chang, Sanghyeon, i Hang Bae Kim. A dark matter solution from the supersymmetric axion model. Office of Scientific and Technical Information (OSTI), maj 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), czerwiec 2004. http://dx.doi.org/10.2172/827002.

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GENERAL THEORY OF THE WHOLE PHYSICAL WORLD. SIB-Expertise, sierpień 2022. http://dx.doi.org/10.12731/er0599.29072022.

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THE WORK CONSISTS IN COMBINING NEWTON'S CLASSICAL MECHANICS DESCRIBED BY EUCLIDIAN GEOMETRY, EINSTEIN'S GENERAL THEORY OF RELATIVITY, QUANTUM MECHANICS, THE THEORY OF SUPERSYMMETRY AND INFLATION THEORY ON THE BASIS OF THE BASIC LAW OF ECONOMIC HEALTH. THE PROPOSED THEORY, INCLUDING ALLOWS TO GIVE ANSWERS TO THE GLOBAL QUESTIONS OF TODAY'S COSMOLOGY AND ASTROPHYSICS: "WHAT WAS BEFORE THE BIG BANG?"; "WHAT IS DARK MATTER?"; "WHAT IS DARK ENERGY?"; “HOW TO UNDERSTAND PARALLEL WORLDS AND MULTI UNIVERSE''. THE WORK WILL SHOW A STRICT CORRELATION OF ALL INTERACTIONS (GRAVITATIONAL, ELECTROMAGNETIC, WEAK AND STRONG) BETWEEN PARTICLES OF MATTER, BOTH ON THE SCALE OF THE GALACTIC SYSTEM AND AT THE LEVEL OF NUCLEI OF ATOMS AND UNSTABLE OUTSIDE ATOMIC NUCLEI OF SUBATOMIC NUCLEI. THESE INTERACTIONS FORMED THE OBSERVABLE PICTURE OF THE WORLD.

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GENERAL THEORY OF THE WHOLE PHYSICAL WORLD. SIB-Expertise, sierpień 2022. http://dx.doi.org/10.12731/er0599.10082022.

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