The Cosmic Neutrino Background is within Reach of Future Neutrino Telescopes

Kavli Affiliate: Shunsaku Horiuchi | Summary:The cosmic neutrino background (C$ν$B) can be boosted to high energies due to scatterings with energetic cosmic rays (CRs) across cosmological scales. Previous calculations focused on neutral current incoherent and coherent elastic scatterings of cosmic-ray protons off relic neutrinos. However, charged current interactions and deep inelastic scatterings are also expected […]


Continue.. The Cosmic Neutrino Background is within Reach of Future Neutrino Telescopes

The Cosmic Neutrino Background is within Reach of Future Neutrino Telescopes

Kavli Affiliate: Shunsaku Horiuchi | Summary:The cosmic neutrino background (C$ν$B) can be boosted to high energies due to scatterings with energetic cosmic rays (CRs) across cosmological scales. Previous calculations focused on neutral current incoherent and coherent elastic scatterings of cosmic-ray protons off relic neutrinos. However, charged current interactions and deep inelastic scatterings are also expected […]


Continue.. The Cosmic Neutrino Background is within Reach of Future Neutrino Telescopes

New Hard X-Ray and Multiwavelength Study of the PeVatron Candidate PWN G0.9+0.1 in the Galactic Center Region

Kavli Affiliate: Melania Nynka | Summary:We present a new X-ray study and multiwavelength spectral energy distribution (SED) modeling of the young pulsar wind nebula (PWN) powered by the energetic pulsar PSR J1747-2809, inside the composite supernova remnant (SNR) G0.9+0.1, located in the Galactic Center region. The source is detected by NuSTAR up to 30 keV […]


Continue.. New Hard X-Ray and Multiwavelength Study of the PeVatron Candidate PWN G0.9+0.1 in the Galactic Center Region

Secret sharing with additive access structures from correlated random variables

Kavli Affiliate: David W. Miller | Summary:We generalize secret-sharing models that rely on correlated randomness and public communication, originally designed for a fixed access structure, to support a sequence of dynamic access structures, which we term an Additive Access Structure. Specifically, the access structure is allowed to monotonically grow by having any subset of participants […]


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OpenVoxel: Training-Free Grouping and Captioning Voxels for Open-Vocabulary 3D Scene Understanding

Kavli Affiliate: Hsiao-Mei (Sherry) Cho| First 5 Authors: [#item_custom_name[1, [#item_custom_name[2, [#item_custom_name[3, [#item_custom_name[4, [#item_custom_name[5| Summary:We propose OpenVoxel, a training-free algorithm for grouping and captioning sparse voxels for the open-vocabulary 3D scene understanding tasks. Given the sparse voxel rasterization (SVR) model obtained from multi-view images of a 3D scene, our OpenVoxel is able to produce meaningful groups […]


Continue.. OpenVoxel: Training-Free Grouping and Captioning Voxels for Open-Vocabulary 3D Scene Understanding

Geometry- and Topology-Informed Quantum Computing: From States to Real-Time Control with FPGA Prototypes

Kavli Affiliate: Hsiao-Mei (Sherry) Cho| First 5 Authors: [#item_custom_name[1, [#item_custom_name[2, [#item_custom_name[3, [#item_custom_name[4, [#item_custom_name[5| Summary:This book gives a geometry-first, hardware-aware route through quantum-information workflows, with one goal: connect states, circuits, and measurement to deterministic classical pipelines that make hybrid quantum systems run. Part 1 develops the backbone (essential linear algebra, the Bloch-sphere viewpoint, differential-geometric intuition, and […]


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The Second CHIME/FRB Catalog of Fast Radio Bursts

Kavli Affiliate: Kiyoshi Masui | Summary:We present a catalog of 4539 fast radio bursts (FRBs) observed with the Canadian Hydrogen Intensity Mapping Experiment (CHIME) telescope between 25 July 2018 and 15 September 2023. These bursts originate from 3641 unique sources, including 981 bursts from 83 known repeating sources. For each FRB, the catalog provides a […]


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NIRPS tightens the mass estimate of GJ 3090 b and detects a planet near the stellar rotation period

Kavli Affiliate: David Charbonneau | Summary:We present an updated characterization of the planetary system orbiting the nearby M2 dwarf GJ 3090 (TOI-177; $d = 22$ pc), based on new high-precision radial velocity (RV) observations from NIRPS and HARPS. With an orbital period of 2.85 d, the transiting sub-Neptune GJ 3090 b has a mass we […]


Continue.. NIRPS tightens the mass estimate of GJ 3090 b and detects a planet near the stellar rotation period

NIRPS tightens the mass estimate of GJ 3090 b and detects a planet near the stellar rotation period

Kavli Affiliate: David Charbonneau | Summary:We present an updated characterization of the planetary system orbiting the nearby M2 dwarf GJ 3090 (TOI-177; $d = 22$ pc), based on new high-precision radial velocity (RV) observations from NIRPS and HARPS. With an orbital period of 2.85 d, the transiting sub-Neptune GJ 3090 b has a mass we […]


Continue.. NIRPS tightens the mass estimate of GJ 3090 b and detects a planet near the stellar rotation period

Light neutrinophilic WIMP in the $U(1)_rm B-L+xY$ model

Kavli Affiliate: Shigeki Matsumoto | Summary:Sub-GeV dark matter is an appealing thermal target because it can still be produced via the standard freeze-out mechanism; at such low masses, achieving freeze-out naturally points to the presence of a light mediator, which shifts the most promising discovery avenues from the energy frontier to the intensity frontier. Realizing […]


Continue.. Light neutrinophilic WIMP in the $U(1)_rm B-L+xY$ model