24,180 research outputs found

    Astrophysical point source search with the ANTARES neutrino telescope

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    The ANTARES neutrino telescope is installed at a depth of 2.5 km of the Mediterranean Sea and consists of a three-dimensional array of 885 photomultipliers arranged on twelve detector lines. The prime objective is to detect high-energy neutrinos from extraterrestrial origin. Relativistic muons emerging from charged-current muon neutrino interactions in the detector surroundings produce a cone of Cerenkov light which allows the reconstruction of the original neutrino direction. The collaboration has implemented different methods to search for neutrino point sources in the data collected since 2007. Results obtained with these methods as well as the sensitivity of the telescope are presented.Comment: 1 page, 1 figur

    Anisotropy of TeV and PeV cosmic rays with IceCube and IceTop

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    The interaction of high energy cosmic rays with the Earth's atmosphere produces extensive air showers of secondary particles with a large muon component. By exploiting the sensitivity of neutrino telescopes to high energy muons, it is possible to use these detectors for precision cosmic ray studies. The high rate of cosmic-ray muon events provides a high-statistics data sample that can be used to look for anisotropy in the arrival directions of the parent particles at the per-mille level. This paper reports on the observation of anisotropy in the cosmic ray data collected with the IceCube neutrino telescope in the 20-400 TeV energy range at multiple angular scales. New data from the IceTop air shower array, located on the ice surface above IceCube, shows an anisotropy that is consistent with the high-energy IceCube results. The sensitivity of IceTop to all the components of the extensive air shower will allow us to explore in more detail the characteristics of the primary cosmic rays associated with the observed anisotropy.Comment: To appear in the Proceedings of the 2011 Very Large Volume Neutrino Telescopes Conferenc

    “Their Image of Me”: A Phenomenological Study of Professional Dress Choices of Female Professors

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    In recent years, scholarly attention to professional dress as a form of nonverbal communication has faded into the background. However, I believe professional dress is an important area of study, considering the changing conditions in the world of work. Therefore, I decided to conduct this phenomenological study of the dress choices of female professors at a small, liberal arts college to discover what professional dress did for them internally and professionally. The analysis of the data suggests that these women try to use dress to represent themselves as who they are internally, without losing sight of their image as a professor, academic, and cultural member. Dress, for them, is a means of controlling and shaping who they view themselves to be into an appropriate external image of who they must be

    Observation of Anisotropy in the Arrival Direction Distribution of Cosmic Rays above TeV Energies with Icecube

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    Between May 2009 and May 2010, the IceCube neutrino detector recorded 32 billion of atmospheric muons generated in air showers produced by cosmic rays in the TeV energy range. With such high statistics sample it is possible to observe, for the first time in the southern hemisphere, an energy dependence in the Galactic cosmic ray anisotropy up to a few hundred TeV. This study shows that the same large-scale anisotropy observed at median energies around 20 TeV is not present at 400 TeV; the anisotropy observed at 400 TeV shows substantial differences with respect to that at lower energy. In addition to the large-scale features observed at 20 TeV in the form of strong dipole and quadrupole moments, the data include several localized regions of excess and deficit on scales between 10{\degree} to 30{\degree}. The features observed at both large and small scale are statistically significant, but their origin is currently unknown.Comment: Proceedings of Rencontres de Blois 201

    The Masculine Sea and the Impossibility of Awakening in Chopin's the Awakening

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    Kate Chopin has a firm place in American women's writing. A persistent theme in her works is said to be women's emotional liberation. The Awakening (1899) as a feminist novel is no exception. In the novel, Edna's inner voice and desire for escape from a male-dominated society awaken in her. Edna's suicide has been interpreted as her victory over the society however, this study argues that the idea of female defeat has been ignored to a great extent the main reason for which is the ignorance or a misreading of sea imagery. The sea of the novel that dissolves Edna is a signifier of male society and language signifying Edna's failure to find a place within the male dialogue of the society. Extra-marital relationships with Alcee or Robert are not promising, for the climax of such relationships is no more than the old requirement of becoming the good wife and mother that the society prescribes to women. By her ultimate suicidal choice, Edna determines to find a voice and be seen but is totally perished instead to prove that women cannot speak. This study intends to argue and conclude that Chopin had this Kristevaesque belief that the male socio-cultural formation does not let women experience freedom. A new interpretation of the sea as a patriarchal element is offered which makes Edna's drowning a total defeat rather than victory as suggested by many critics

    IceCube: physics, status, and future

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    The IceCube observatory is the first cubic kilometre scale instrument in the field of high-energy neutrino astronomy and cosmic rays. In 2009, following five successful deployment seasons, IceCube consisted of 59 strings of optical modules in the South Pole ice, together with 118 air shower detectors in the IceTop surface array. The range of physics topics includes neutrino signals from astrophysical sources, dark matter, exotic particle physics, cosmic rays, and atmospheric neutrinos. The current IceCube status and selected results are described. Anticipated future developments are also discussed, in particular the Deep Core low energy subarray which was recently deployed.Comment: Presentation at the 4th International Workshop on Very Large Volume Neutrino Telescope

    Polarized and Unpolarized Lepton Pair Forward-backward Asymmetries in BK0(1430)+\overline{B}\rightarrow \overline{K}_{0}^{*}(1430) \ell^+\ell^- and BK+\overline{B}\rightarrow \overline{K} \ell^+\ell^- Decays in Two Higgs Doublet Model

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    In this paper we shall focus on the effects of concrete models such as SM and Model III of 2HDM on the polarized and unpolarized forward-backward asymmetries of BK0(1430)+\overline{B}\rightarrow \overline{K}_0^{*}(1430) \ell^+\ell^- and BK+\overline{B}\rightarrow \overline{K} \ell^+\ell^- decays. The obtained results of these decay modes are compared to each other. Also, we obtain the minimum required number of events for detecting each asymmetry and compare them with the number of produced BBˉB\bar{B} pairs at the LHC or supposed to be produced at the Super-LHC. At the end, we conclude that the study of these asymmetries for BK0(1430)+\overline{B}\rightarrow \overline{K}_0^*(1430) \ell^+\ell^- and BK+\overline{B}\rightarrow \overline{K} \ell^+\ell^- processes are very effective tools for establishing new physics in the future B-physics experiments

    Dissipative Charged Fluid in a Magnetic Field

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    We study the collective excitations in a dissipative charged fluid at zero chemical potential when an external magnetic field is present. While in the absence of magnetic field, four collective excitations appear in the fluid, we find five hydrodynamic modes in presence of magnetic field. This implies that the magnetic field splits the degeneracy between the transverse shear modes. Using linear response theory, we then compute the retarded response functions. In particular, it turns out that the correlation between charge and the energy fluctuations will no longer vanish, even at zero chemical potential. By use of the response functions, we also derive the relevant Kubo formulas for the transport coefficients.Comment: 6 page
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