2,403 research outputs found

    Naturalness of Neutralino Dark Matter

    Full text link
    We investigate the level of fine-tuning of neutralino Dark Matter below 200 GeV in the low-energy phenomenological minimal supersymmetric Standard Model taking into account the newest results from XENON100 and the Large Hadron Collider as well as all other experimental bounds from collider physics and the cosmological abundance. We find that current and future direct Dark Matter searches significantly rule out a large area of the untuned parameter space, but solutions survive which do not increase the level of fine-tuning. As expected, the level of tuning tends to increase for lower cross-sections, but regions of resonant neutralino annihilation still allow for a band at light masses, where the fine-tuning stays small even below the current experimental limits for direct detection cross-sections. For positive values of the supersymmetric Higgs mass parameter \mu large portions of the allowed parameter space are excluded, but there still exist untuned solutions at higher neutralino masses which will essentially be ruled out if XENON1t does not observe a signal.For negative \mu untuned solutions are not much constrained by current limits of direct searches and, if the neutralino mass was found outside the resonance regions, a negative \mu-term would be favored from a fine-tuning perspective. Light stau annihilation plays an important role to fulfill the relic density condition in certain neutralino mass regions. Finally we discuss, in addition to the amount of tuning for certain regions in the neutralino mass-direct detection cross-section plane, the parameter mapping distribution if the allowed model parameter space is chosen to be scanned homogeneously (randomized).Comment: v2: 29 pages, 16 figures. Published versio

    Filme drehen im Fremdsprachenunterricht

    Get PDF

    From the Cooper problem to canted supersolids in Bose-Fermi mixtures

    Get PDF
    We calculate the phase diagram of the Bose-Fermi Hubbard model on the 3d cubic lattice at fermionic half filling and bosonic unit filling by means of single-site dynamical mean-field theory. For fast bosons, this is equivalent to the Cooper problem in which the bosons can induce s-wave pairing between the fermions. We also find miscible superfluid and canted supersolid phases depending on the interspecies coupling strength. In contrast, slow bosons favor fermionic charge density wave structures for attractive fermionic interactions. These competing instabilities lead to a rich phase diagram within reach of cold gas experiments.Comment: 5 pages, 4 figures; replaced with published versio

    Strongly Monotone Drawings of Planar Graphs

    Get PDF
    A straight-line drawing of a graph is a monotone drawing if for each pair of vertices there is a path which is monotonically increasing in some direction, and it is called a strongly monotone drawing if the direction of monotonicity is given by the direction of the line segment connecting the two vertices. We present algorithms to compute crossing-free strongly monotone drawings for some classes of planar graphs; namely, 3-connected planar graphs, outerplanar graphs, and 2-trees. The drawings of 3-connected planar graphs are based on primal-dual circle packings. Our drawings of outerplanar graphs are based on a new algorithm that constructs strongly monotone drawings of trees which are also convex. For irreducible trees, these drawings are strictly convex

    Conformal Little Higgs

    Full text link
    Little Higgs models address the hierarchy problem by identifying the SM Higgs doublet as pseudo-Nambu--Goldstone bosons (pNGB) arising from global symmetries with collective breakings. These models are designed to address the little hierarchy problem up to a scale of Λ ⁣ ⁣O(10) \Lambda\!\sim\! {\cal O}(10)~TeV. Consequently, these models necessitate an ultraviolet (UV) completion above this scale. On the other hand, conformal extensions of the Standard Model are intriguing because scales emerge as a consequence of dimensional transmutation. In this study, we present a unified framework in which the electroweak hierarchy problem is tackled through a conformal symmetry collectively broken around the TeV scale, offering an appealing UV completion for Little Higgs models. Notably, this framework automatically ensures the presence of the required UV fixed points, eliminating the need for careful adjustments to the particle content of the theory. Moreover, this framework naturally addresses the flavor puzzles associated with composite or Little Higgs models. Furthermore, we suggest that in this framework all known Little Higgs models can be UV-completed through conformal dynamics above the scale Λ\Lambda up to arbitrary high scales.Comment: 8 page

    Weak Factors are Everywhere

    Full text link
    Factor Sequences are stochastic double sequences indexed in time and cross-section which have a so called factor structure. The term was coined by Forni and Lippi (2001) who introduced dynamic factor sequences. We introduce the distinction between dynamic- and static factor sequences which has been overlooked in the literature. Static factor sequences, where the static factors are modeled by a dynamic system, are the most common model of macro-econometric factor analysis, building on Chamberlain and Rothschild (1983a); Stock and Watson (2002a); Bai and Ng (2002). We show that there exist two types of common components - a dynamic and a static common component. The difference between those consists of the weak common component, which is spanned by (potentially infinitely many) weak factors. We also show that the dynamic common component of a dynamic factor sequence is causally subordinated to the output under suitable conditions. As a consequence only the dynamic common component can be interpreted as the projection on the infinite past of the common innovations of the economy, i.e. the part which is dynamically common. On the other hand the static common component captures only the contemporaneous co-movement
    corecore