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  1. 5381
    “…The effective interaction strength is constrained by the SM precision measurements, astrophysical and cosmological observations. We introduce a novel effective electromagnetic interaction between sterile neutrinos and SM neutrinos, which can successfully explain the XENON1T event rate through inelastic scattering of the sterile neutrino dark matter from Xenon electrons. …”
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    Shedding new light on sterile neutrinos from XENON1T experiment
  2. 5382
    “…We use robust combinations of different cosmological observations, namely the Cosmic Microwave Background (CMB), local measurement of Hubble constant ([Formula: see text]), Baryon Acoustic Oscillation (BAO) and SnIa for this purpose. …”
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    Dark Energy with Phantom Crossing and the H(0) Tension
  3. 5383
    por Vanchurin, Vitaly
    Publicado 2021
    “…We show that the non-equilibrium dynamics of non-trainable variables can be described by the geodesic equation (in the emergent space-time) for localized states of neurons, and by the Einstein equations (with cosmological constant) for the entire network. We conclude that the quantum description of trainable variables and the gravitational description of non-trainable variables are dual in the sense that they provide alternative macroscopic descriptions of the same learning system, defined microscopically as a neural network.…”
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    Online Artículo Texto
    Towards a Theory of Quantum Gravity from Neural Networks
  4. 5384
    “…First, we show how Haredi cosmologies and culture come together to critique science as an epistemology while engaging with science as a technology. …”
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    Online Artículo Texto
    “We think this way as a society!”: Community-level science literacy among ultra-Orthodox Jews
  5. 5385
    “…The experimental upper limit on the electric dipole moment of the electron could be reconciled with leptogenesis, if the latter occurs at a relatively low scale, which would also alleviate the cosmological gravitino problem. Even if lepton non-universality is not seen…”
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    Supersymmetric Grand Unification and Lepton Universality in $K \to l\nu$ Decays
  6. 5386
    “…We have performed a number of dark matter only simulations from cosmological initial conditions inside boxes with sizes from 1 to 4 Mpc. …”
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    Overcooled haloes at z ≥ 10: a route to form low-mass first stars
  7. 5387
    “…Large scale structure surveys promise to be the next leading probe of cosmological information. It is therefore crucial to reliably predict their observables. …”
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    The Effective Field Theory of Large Scale Structures at Two Loops
  8. 5388
    por Mavromatos, Nick E.
    Publicado 2014
    “…More specifically, after reviewing some generic models of background-induced CPTV in early epochs of the Universe, we consider a string-inspired scenario, in which the CPTV is associated with a cosmological background with torsion provided by the Kalb-Ramond (KR) antisymemtric tensor field of the string gravitational multiplet. …”
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    Pseudoscalar Fields in Torsionful Geometries of the Early Universe, the Baryon Asymmetry and Majorana Neutrino Mass Generation
  9. 5389
    “…We also implement CP-conserving constraints from Higgs physics, flavour physics and the upper limits on the cosmological dark matter density and spin-independent scattering. …”
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    Exploring CP Violation in the MSSM
  10. 5390
    “…We consider a class of models with gauged U(1)_R symmetry in 4D N=1 supergravity that have, at the classical level, a metastable ground state, an infinitesimally small (tunable) positive cosmological constant and a TeV gravitino mass. We analyse if these properties are maintained under the addition of visible sector (MSSM-like) and hidden sector state(s), where the latter may be needed for quantum consistency. …”
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    Gauged R-symmetry and its anomalies in 4D N=1 supergravity and phenomenological implications
  11. 5391
    por Khlopov, Maxim Yu., Kouvaris, Chris
    Publicado 2007
    “…Minimal walking technicolor models can provide a nontrivial solution for cosmological dark matter, if the lightest technibaryon is doubly charged. …”
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    Strong Interactive Massive Particles from a Strong Coupled Theory
  12. 5392
    por Ellis, John R., King, S.F., Roberts, J.P.
    Publicado 2007
    “…We study the amounts of fine-tuning of the parameters of the MSSM with non-universal soft supersymmetry-breaking contributions to the Higgs masses (the NUHM) that would be required for the relic neutralino density to lie within the range favoured by WMAP and other astrophysical and cosmological observations. Such dark matter fine-tuning is analogous to the commonly studied electroweak fine-tuning associated with satisfying the electroweak symmetry breaking conditions, which we also study for completeness. …”
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    The Fine-Tuning Price of Neutralino Dark Matter in Models with Non-Universal Higgs Masses
  13. 5393
    por McElrath, Bob
    Publicado 2009
    “…One can describe cosmological relic neutrinos by adding Lagrange multipliers to the Standard Model Lagrangian for them. …”
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    On The Origin of Neutrino Mass and Mixing in the Standard Model
  14. 5394
    “…We construct explicit new physics models that give an order one (or larger) increase of photon count in the RJ tail, which can be tested by existing and upcoming experiments aiming to detect the cosmological 21 cm emission or absorption signal. This class of models stipulates the decay of unstable particles to dark photons A′ that have a small mass, mA′∼10-14–10-9  eV, nonvanishing mixing angle ε with electromagnetism, and energies much smaller than TCMB. …”
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    Room for New Physics in the Rayleigh-Jeans Tail of the Cosmic Microwave Background
  15. 5395
    “…However, the 0-point energy left over from the epoch of large photon mass may have persisted, during the post-inflationary universe, as very weak, but cosmological-scale, magnetic fields. It has been suggested that these small, seed fields were amplified by a dynamo mechanism to produce the micro-Gauss magnetic fields observed in galaxies and galactic clusters.…”
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    Vacuum polarization and photon mass in inflation
  16. 5396
    por McElrath, Bob
    Publicado 2008
    “…We show that any massive cosmological relic particle with small self-interactions is a super-fluid today, due to the broadening of its wave packet, and lack of any elastic scattering. …”
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    Emergent Electroweak Gravity
  17. 5397
    “…We analyze the parameter space of CFSU(5) assuming that the lightest supersymmetric particle (LSP) provides the cosmological cold dark matter, paying careful attention to the matching of parameters at the GUT scale. …”
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    Constrained Supersymmetric Flipped SU(5) GUT Phenomenology
  18. 5398
    por Aune, S., Barth, K., Belov, A., Borghi, S., Brauninger, H., Cantatore, G., Carmona, J.M., Cetin, S.A., Collar, J.I., Dafni, T., Davenport, M., Eleftheriadis, C., Elias, N., Ezer, C., Fanourakis, G., Ferrer-Ribas, E., Friedrich, P., Galan, J., Garcia, J.A., Gardikiotis, A., Gazis, E.N., Geralis, T., Giomataris, I., Gninenko, S., Gomez, H., Gruber, E., Guthorl, T., Hartmann, R., Haug, F., Hasinoff, M.D., Hoffmann, D.H.H., Iguaz, F.J., Irastorza, I.G., Jacoby, J., Jakovcic, K., Karuza, M., Konigsmann, K., Kotthaus, R., Krcmar, M., Kuster, M., Lakic, B., Laurent, J.M., Liolios, A., Ljubicic, A., Lozza, V., Lutz, G., Luzon, G., Morales, J., Niinikoski, T., Nordt, A., Papaevangelou, T., Pivovaroff, M.J., Raffelt, G., Rashba, T., Riege, H., Rodriguez, A., Rosu, M., Ruz, J., Savvidis, I., Silva, P.S., Solanki, S.K., Stewart, L., Tomas, A., Tsagri, M., van Bibber, K., Vafeiadis, T., Villar, J.A., Vogel, J.K., Yildiz, S.C., Zioutas, K.
    Publicado 2011
    “…In future we will extend our search to m_a < 1.15 eV, comfortably overlapping with cosmological hot dark matter bounds.…”
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    CAST search for sub-eV mass solar axions with $^{3}$He buffer gas
  19. 5399
    por Conrad, Jan
    Publicado 2012
    “…Predictions for the next generation air Cherenkov telescope, Cherenkov Telescope Array (CTA), together with forecasts on future Fermi-LAT constraints arrive at the exciting possibility that the cosmological benchmark cross-section could be probed from masses of a few GeV to a few TeV. …”
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    Searches for Particle Dark Matter with gamma-rays.
  20. 5400
    por Kostelecký, V Alan
    Publicado 2014
    “…Topics covered at the meeting include searches for CPT and Lorentz violations involving: accelerator and collider experiments; atomic, nuclear, and particle decays; birefringence, dispersion, and anisotropy in cosmological sources; clock-comparison measurements; electromagnetic resonant cavities and lasers; tests of the equivalence principle; gauge and Higgs particles; high-energy astrophysical observations; laboratory tests of gravity; matter interferometry; neutrino oscillations and propagation; oscillations and decays of neutral mesons; particle–antiparticle comparisons; post-newtonian gravity in the solar system and beyond; second- and third-generation particles; space-based missions; spectroscopy of hydrogen and antihydrogen; spin-polarized matter; and time-of-flight measurements. …”
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    Sixth Meeting on CPT and Lorentz Symmetry
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