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arXiv:2406.19262 (Published 2024-06-27)
A Short Note on the Love Number of Extremal Reissner-Nordstrom and Kerr-Newman Black Holes
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arXiv:2406.19284 (Published 2024-06-27)
Interacting ultralight dark matter and dark energy and fits to cosmological data in a field theory approach
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arXiv:2406.19287 (Published 2024-06-27)
Isotropy of cosmic rays beyond $10^{20}$ eV favors their heavy mass composition
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arXiv:2406.19264 (Published 2024-06-27)
A rare, strong shock front in the merging cluster SPT-CL J2031-4037
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arXiv:2406.19337 (Published 2024-06-27)
A Contact Binary Satellite of the Asteroid (152830) Dinkinesh
Harold F. Levison, Simone Marchi, Keith S. Noll, John R. Spencer, Thomas S. Statler, the Lucy mission teamCategories: astro-ph.EPKeywords: first confirmed contact binary satellite, prominent longitudinal trough overlain, main asteroid belt, heliocentric semimajor axis, substantial equatorial ridgeTags: journal article -
arXiv:2406.19286 (Published 2024-06-27)
Mass composition of ultra-high energy cosmic rays from distribution of their arrival directions with the Telescope Array
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arXiv:2406.19355 (Published 2024-06-27)
A class of ghost-free theories in symmetric teleparallel geometry
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arXiv:2406.19210 (Published 2024-06-27)
The Maclaurin spheroid in disguise. New figures of equilibrium with external magnetic support
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arXiv:2406.19184 (Published 2024-06-27)
The Lyman-limit photon mean free path at the end of late reionisation in the Sherwood-Relics simulations
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arXiv:2406.19177 (Published 2024-06-27)
Stability of the Potential Super Jupiter in Alpha Centauri System
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arXiv:2406.19199 (Published 2024-06-27)
The case for Centaurus A as the main source of ultrahigh-energy cosmic rays
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arXiv:2406.19233 (Published 2024-06-27)
X-ray and gamma-ray study for 2023 nova eruption of V1716 Sco
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arXiv:2406.19295 (Published 2024-06-27)
M31 nucleus: molecular and ionised gas content upper limits
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arXiv:2406.19279 (Published 2024-06-27)
Probing self-interacting ultra-high-energy neutrinos with cosmic 21-cm signal
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arXiv:2406.19367 (Published 2024-06-27)
PUREPath: A Deep Latent Variational Model for Estimating CMB Posterior over Large Angular Scales of the Sky
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arXiv:2406.19385 (Published 2024-06-27)
A Machine Learning Method for Monte Carlo Calculations of Radiative Processes
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arXiv:2406.19274 (Published 2024-06-27)
Preserving quantum information in $f(Q)$ cosmology
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arXiv:2406.19375 (Published 2024-06-27)
Calibrating and standardizing the Tip of the Red Giant Branch in the Small Magellanic Cloud using small-amplitude red giants
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arXiv:2406.19218 (Published 2024-06-27)
Rotation curves velocities obtained by warm low-density plasma simulating dark halos and dark matter
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arXiv:2406.19229 (Published 2024-06-27)
Diffuse interstellar bands in the near-infrared: Expanding the reddening range