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  1. 5421
    por Calfayan, P
    Publicado 2014
    “…Multiple cosmological observations indicate the existence of Dark Matter, which may be a weakly interacting massive particle (WIMP). …”
    Enlace del recurso
    Dark Matter searches at the LHC
  2. 5422
    “…We show that current bounds on these effective parameters do not vary significantly when considering an arbitrary value of the particle mass, or extended cosmological models with a free effective neutrino number, dynamical dark energy or a running of the primordial spectrum tilt. …”
    Enlace del recurso
    Enlace del recurso
    Robustness of cosmic neutrino background detection in the cosmic microwave background
  3. 5423
    “…Similarly, evanescent fields do not propagate in D=4; a three-form field is in this class, since it is dual to a cosmological-constant contribution. In this Letter, we show that evanescent operators and fields modify the leading ultraviolet divergence in pure gravity. …”
    Enlace del recurso
    Enlace del recurso
    Evanescent Effects Can Alter Ultraviolet Divergences in Quantum Gravity without Physical Consequences
  4. 5424
    Publicado 2016
    “…Probing this structure or observing any deviation will have long-reaching implications on our understanding on how Nature works at its most fundamental level, including connections with other cosmological problems. The primary goal of this workshop is to bring together experts from the theoretical and experimental communities for a joint brainstorming on the status of this research, identify areas for improvements, as well as set new promising directions to be confronted with the first LHC data at 13 TeV.…”
    Enlace del recurso
    Higgs Tasting Workshop 2016: Higgs and flavor in the LHC Run 2 era
  5. 5425
    por Mielke, Eckehard W
    Publicado 2016
    “…After symmetry breaking, Einstein’s standard general relativity with cosmological constant emerges as a classical background. …”
    Enlace del recurso
    Enlace del recurso
    Geometrodynamics of gauge fields: on the geometry of Yang-Mills and gravitational gauge theories
  6. 5426
    “…The notions of asymptotically flat spacetimes and of expanding universes with a cosmological horizon are analysed in detail, devoting special attention to the characterization of asymptotic symmetries. …”
    Enlace del recurso
    Enlace del recurso
    Hadamard states from light-like hypersurfaces
  7. 5427
    por Valle, Nicolo'
    Publicado 2021
    “…The interest in the phenomenology of relativistic heavy-ion collisions is driven by the many open points about the nature of the strong interaction, as well as by cosmological reasons. The physics of heavy ions is not limited to the study of the hot matter created when they collide (QGP, Quark-Gluon Plasma); the nuclear environment modifies the behaviour of their constituents independently on the subsequent QGP formation. …”
    Enlace del recurso
    Measuring Z boson production in heavy-ion collisions with ALICE, with a view on the upgrade of the experiment
  8. 5428
    “…Dark matter is a key piece of the current cosmological scenario, with weakly interacting massive particles (WIMPs) a leading dark matter candidate. …”
    Enlace del recurso
    Enlace del recurso
    Search for Ultraheavy Dark Matter from Observations of Dwarf Spheroidal Galaxies with VERITAS
  9. 5429
    “…The rates are promisingly large when the soft supersymmetry-breaking mass parameters are chosen to be consistent with the cosmological relic-density constraints. In addition, we discuss mu -> e conversion on Titanium, which may also be accessible to future experiments.…”
    Enlace del recurso
    Enlace del recurso
    Charged-lepton-flavour violation in the light of the super-Kamiokande data
  10. 5430
    por Szalay, Alexander S., Jain, Bhuvnesh, Matsubara, Takahiko, Scranton, Ryan, Vogeley, Michael S., Connolly, Andrew, Dodelson, Scott, Eisenstein, Daniel, Frieman, Joshua A., Gunn, James E., Hui, Lam, Johnston, David, Kent, Stephen M., Kerscher, Martin, Loveday, Jon, Meiksin, Avery, Narayanan, Vijay, Nichol, Robert C., O'Connell, Liam, Pope, Adrian, Scoccimarro, Roman, Sheth, Ravi K., Stebbins, Albert, Strauss, Michael A., Szapudi, Istvan, Tegmark, Max, Zehavi, Idit, Annis, James, Bahcall, Neta A., Brinkmann, Jon, Csabai, Istvan, Fukugita, Masataka, Hennessy, Greg, Hogg, David W., Ivezic, Zeljko, Knapp, Gillian R., Kunszt, Peter Z., Lamb, Don Q., Lee, Brian C., Lupton, Robert H., Munn, Jeffrey R., Peoples, John, Pier, Jeffrey R., Rockosi, Constance, Schlegel, David, Stoughton, Christopher, Tucker, Douglas L., Yanny, Brian, York, Donald G.
    Publicado 2001
    “…Our best estimates are Gamma=0.188 +/- 0.04 and sigma_8L = 0.915 +/- 0.06 (statistical errors only), for a flat Universe with a cosmological constant. We demonstrate that our measurements contain signal from scales at or beyond the peak of the 3D power spectrum. …”
    Enlace del recurso
    Enlace del recurso
    KL Estimation of the Power Spectrum Parameters from the Angular Distribution of Galaxies in Early SDSS Data
  11. 5431
    “…We find actually that for m^4 / lambda = 50 - 75 eV^4, the agreement with the measurements of the circular speed of DDO 154 is impressive whereas it lessens for larger systems. The cosmological behavior of the field is also found to be consistent - yet marginally - with the limits set by BBN on the effective number of neutrino families. …”
    Enlace del recurso
    Enlace del recurso
    Galactic Halos of Fluid Dark Matter
  12. 5432
    “…We identify the general mechanism for and limitations of the self-tuning of the effective 4D cosmological constant in higher-dimensional supergravity which these models illustrate.…”
    Enlace del recurso
    Enlace del recurso
    Warped Brane Worlds in Six Dimensional Supergravity
  13. 5433
    por Heinemeyer, S, Hollik, W, Weiglein, Georg
    Publicado 2004
    “…The mSUGRA scenario with cosmological constraints yields a very good fit to the data, showing a clear preference for a relatively light mass scale of the SUSY particles. …”
    Enlace del recurso
    Enlace del recurso
    Electroweak Precision Observables in the Minimal Supersymmetric Standard Model
  14. 5434
    “…Can MPP Together with Weinberg-Salam Higgs Provide Cosmological Inflation? (D.L. Bennett and H.B. Nielsen) 2. …”
    Enlace del recurso
    8th Workshop on What Comes Beyond the Standard Model
  15. 5435
    por Gustavino, Giuliano
    Publicado 2017
    “…Many cosmological observations indicate that the matter predicted and described by the Standard Model constitutes only a small fraction of the entire known universe. …”
    Enlace del recurso
    Enlace del recurso
    Search for New Physics in Mono-jet Final States in pp Collisions at √s = 13 TeV with the ATLAS Experiment at the LHC
  16. 5436
    por De Lellis, Giovanni
    Publicado 2001
    “…The design has been optimized to explore the $\Delta m^2$ region of cosmological interest in relation to the Dark Matter in a high $sin^2(2\theta)$ sensitivity. …”
    Enlace del recurso
    A Search For $\nu_{\mu} \to \nu_{\tau}$ Oscillations In CHORUS
  17. 5437
    “…The DGRB possibly encompasses contributions from different source populations such as star-forming galaxies, starburst galaxies, active galactic nuclei, gamma-ray bursts, or galaxy clusters. Here, we combine cosmological magnetohydrodynamical simulations of clusters of galaxies with the propagation of cosmic rays (CRs) using Monte Carlo simulations, in the redshift range z ≤ 5.0, and show that the integrated gamma-ray flux from clusters can contribute up to 100% of the DGRB flux observed by Fermi-LAT above 100 GeV, for CRs spectral indices α = 1.5 − 2.5 and energy cutoffs [Formula: see text] eV. …”
    Enlace del recurso
    Enlace del recurso
    Enlace del recurso
    Online Artículo Texto
    The diffuse gamma-ray flux from clusters of galaxies
  18. 5438
    “…Through co-annihilations, models of inelastic dark matter (iDM) and inelastic Dirac dark matter (i2DM) can reproduce the observed relic density in the MeV to GeV mass range without violating cosmological limits. In these scenarios, the vector mediator behaves like a semi-visible particle, evading traditional bounds on visible or invisible resonances, and uncovering new parameter space to explain the muon [Formula: see text] anomaly. …”
    Enlace del recurso
    Enlace del recurso
    Enlace del recurso
    Online Artículo Texto
    Constraining light thermal inelastic dark matter with NA64
  19. 5439
    “…Supposing that the Universe contains also the cosmological constant and a perfect fluid with a negative constant equation of state (EoS) parameter [Formula: see text] (e.g., quintessence, phantom or frustrated network of topological defects), we investigate scalar perturbations of the Friedmann–Robertson–Walker metrics due to inhomogeneities. …”
    Enlace del recurso
    Enlace del recurso
    Enlace del recurso
    Online Artículo Texto
    Rigorous theoretical constraint on constant negative EoS parameter [Formula: see text] and its effect for the late Universe
  20. 5440
    por Markkanen, T.
    Publicado 2018
    “…In contrast to the usual semi-classical prescription, as the source term in the Friedmann equations we use expectation values where the unobservable information hidden by the cosmological event horizon has been neglected i.e. coarse grained over. …”
    Enlace del recurso
    Enlace del recurso
    Enlace del recurso
    Online Artículo Texto
    De Sitter stability and coarse graining
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