Suggested Topics within your search.
Suggested Topics within your search.
- Physics 1
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561
On the novel nonlinear propagating waves in stochastic dispersive mode
Published 2025-03-01“…It was observed that noise effects might alter the wave characteristics, thereby producing unprecedented physical and astrophysical densities.…”
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562
Signature of Plausible Accreting Supermassive Black Holes in Mrk 261/262 and Mrk 266
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563
Primordial black holes and their gravitational-wave signatures
Published 2025-01-01“…Significant progress has been achieved both on the theory side and from the point of view of observations, including new models and more accurate calculations of PBH formation, evolution, clustering, merger rates, as well as new astrophysical and cosmological probes. In this work, we review, analyze and combine the latest developments in order to perform end-to-end calculations of the various gravitational-wave signatures of PBHs. …”
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564
Curvature-Restored Gauge Invariance and Ultraviolet Naturalness
Published 2016-01-01“…It can source various cosmological, astrophysical, and collider phenomena depending on its spectrum and couplings to the SM.…”
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565
The DarkSide Multiton Detector for the Direct Dark Matter Search
Published 2015-01-01“…Although the existence of dark matter is supported by many evidences, based on astrophysical measurements, its nature is still completely unknown. …”
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566
Production of Oxidants by Ion Bombardment of Icy Moons in the Outer Solar System
Published 2011-01-01“…Our groups in Brazil, France and Italy have been active, among others in the world, in performing experiments on physical-chemical effects induced by fast ions colliding with solids (frozen gases, carbonaceous and organic materials, silicates, etc.) of astrophysical interest. The used ions span a very large range of energies, from a few keV to hundreds MeV. …”
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567
Dark Atoms and the Positron-Annihilation-Line Excess in the Galactic Bulge
Published 2014-01-01“…The cross-section for OHe collisions with excitation to 2s level is calculated and it is shown that the rate of such excitations in the galactic bulge strongly depends not only on the mass of O-helium, which is determined by the mass of O--, but also on the density and velocity distribution of dark matter. Given the astrophysical uncertainties on these distributions, this mechanism constrains the O-- mass to lie in two possible regions. …”
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568
Complements to the Theoretical Treatments of the Electron Collision with : An R-Matrix Approach
Published 2013-01-01“…To the best of our knowledge, the work reported herein describes for the first time a detailed calculation for this atomic system, and the results are relevant to the laboratory and astrophysical plasmas.…”
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569
Relating quantum mechanics and kinetics of neutrino oscillations
Published 2020-01-01“…Abstract Simultaneous treatment of neutrino oscillations and collisions in astrophysical environments requires the use of (quantum) kinetic equations. …”
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570
Charged superradiant instability in a spherical regular black hole
Published 2024-12-01“…This growth rate significantly exceeds the instability identified in ABG black holes discussed in prior research, suggesting a notable timescale for detecting this phenomenon in astrophysical scenarios. Additionally, we conduct a thorough investigation into how the three parameters of the model influence the onset and intensity of the instability. …”
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571
Lorentz violation alleviates gravitationally induced entanglement degradation
Published 2025-01-01“…This suggests that investigating Lorentz violation at astrophysical scales requires low-frequency detectors, as the low energy of these fields enhances the significance of the Lorentz-violating field’s non-zero vacuum expectation value.…”
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572
Analysis of coupled acoustic and drift modes leading to modons in Maxwellian and non-Maxwellian dusty plasma
Published 2025-01-01“…Numerical analysis shows the formation of vortices is impacted by nonthermality. The astrophysical and laboratory contexts provide a useful perspective on the significance of this analysis.…”
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573
Analyzing the speed of sound in neutron star with machine learning
Published 2024-12-01“…In this work, we use a neural network approach to study matter at intermediate densities to analyze the variation of the speed of sound and the measure of trace anomaly considering astrophysical constraints of mass–radius measurement of 18 neutron stars. …”
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574
The hierarchical three-body problem at O G 2 $$ \mathcal{O}\left({G}^2\right) $$
Published 2025-01-01“…Our results are exact in velocity, and can be used in analyses involving both bound and unbound hierarchical triples in astrophysical systems.…”
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575
The Discreet Charm of Higgsino Dark Matter: A Pocket Review
Published 2018-01-01“…In the second part we properly review the prospects for detection of a higgsino-like neutralino in direct underground dark matter searches, collider searches, and indirect astrophysical signals. We provide estimates for the typical scale of the superpartners and fine tuning in the context of traditional scenarios where the breaking of supersymmetry is mediated at about the scale of Grand Unification and where strong expectations for a timely detection of higgsinos in underground detectors are closely related to the measured 125 GeV mass of the Higgs boson at the LHC.…”
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576
Internal gravity waves versus inertial waves in the laboratory
Published 2024-11-01“…Density-stratified and/or rotating fluids are very common in geophysical and astrophysical flows and enable the propagation of respectively internal gravity waves and inertial waves. …”
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577
Enhancing Solar Convection Analysis With Multi‐Core Processors and GPUs
Published 2025-01-01“…ABSTRACT In the realm of astrophysical numerical calculations, the demand for enhanced computing power is imperative. …”
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578
Quasi-biennial oscillation: laboratory experiments
Published 2024-09-01“…This wind is a mean flow induced by atmospheric waves, including internal gravity waves, which explain that the period (28 month) is not linked to any astrophysical forcing. This oscillation has only been reproduced in 3 laboratory experiments, which share a similar geometry. …”
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579
Models of Anisotropic Self-Gravitating Source in Einstein-Gauss-Bonnet Gravity
Published 2018-01-01“…Each solution can be represented in term of arbitrary function of time; this function has been chosen arbitrarily to fit the different astrophysical time profiles. The existing solutions forecast gravitational expansion and collapse depending on the choice of initial data. …”
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580
Herrera complexity and shadows of spherically symmetric compact objects
Published 2025-02-01“…In this context we explore how complexity of compact objects (a fundamentally theoretical classification) is connected to the photon ring (an astrophysical observable in the universe) and its stability. …”
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