Warm, not Fuzzy: Generalized Ultralight Dark Matter Limits from Milky Way Satellites

Kavli Affiliate: Risa Wechsler | Summary:We generalize lower limits on the dark matter (DM) particle mass $m$ derived from Milky Way (MW) satellite galaxy abundances to scenarios in which DM is an ultralight scalar field produced with a field power spectrum peaked at a subhorizon wavenumber $k_*$. In these models, the DM field free-streams similar […]


Continue.. Warm, not Fuzzy: Generalized Ultralight Dark Matter Limits from Milky Way Satellites

Opportunities for Gravitational Wave Physics at the South Pole

Kavli Affiliate: Peter Graham | Summary:Atom interferometers represent a promising approach for gravitational wave detection in the decihertz frequency band, complementary to existing light-based detectors. The South Pole offers unique advantages for such experiments: exceptionally low seismic noise, established infrastructure for large scientific projects, and a location that strengthens gravitational wave source localization through global […]


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Smaller Than Earth Habitability Model (STEHM): The Lower Size Limit for Atmosphere Retention in the Habitable Zone

Kavli Affiliate: Laura Schaefer | Summary:With recent advances in exoplanet observational techniques enabling the discovery of increasingly smaller planets, a crucial question emerges in the search for habitable planets: how small can a planet be and still maintain an atmosphere? We present results from the Smaller Than Earth Habitability Model (STEHM) which examines how small […]


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Self-consistent numerical simulations for the formation and dynamics of solar prominences

Kavli Affiliate: Robert Cameron | Summary:Solar prominences are cool and dense plasma structures floating in the hot solar corona. They are ubiquitous features in the solar atmosphere, but their formation mechanism is still unclear. Here we perform comprehensive fully three-dimensional numerical simulations of prominence formation including the physics necessary to describe all atmospheric layers of […]


Continue.. Self-consistent numerical simulations for the formation and dynamics of solar prominences

The dark and featureless surface of rocky exoplanet LHS 3844 b from JWST mid-infrared spectroscopy

Kavli Affiliate: Laura Schaefer | Summary:JWST has opened a new era in the study of rocky exoplanets, enabling direct characterization of their surfaces with mid-infrared spectroscopy. Different types of rock have distinct spectral features that are diagnostic of the chemical composition and other physical properties like surface texture. Measurements of these features can provide valuable […]


Continue.. The dark and featureless surface of rocky exoplanet LHS 3844 b from JWST mid-infrared spectroscopy

Itô tracers: continuous-trajectory Lagrangian particles for Eulerian hydrodynamics

Kavli Affiliate: Tom Abel | Summary:Lagrangian tracer particles have long been used to track the history of individual gas parcels in hydrodynamical codes. Particles advected by the cell-centered velocity carry no representation of underlying numerical diffusion, and thus exhibit systematic bias. The Monte-Carlo (MC) tracer resolves this with discrete probabilistic cell-to-cell, flux-based jumps, at the […]


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IXPE Polarizations of the Lighthouse Pulsar, Trail, and Filament

Kavli Affiliate: Roger Romani | Summary:The Lighthouse pulsar (PSR J1101$-$6101) sports a bright X-ray trail and filament. The synchrotron emission from both structures is expected to be polarized, with electric vector position angle (EVPA) perpendicular to the magnetic field direction and polarization degree (PD) indicating the local degree of magnetic turbulence. We present a 1 […]


Continue.. IXPE Polarizations of the Lighthouse Pulsar, Trail, and Filament

IXPE Polarizations of the Lighthouse Pulsar, Trail, and Filament

Kavli Affiliate: Roger Romani | Summary:The Lighthouse pulsar (PSR J1101$-$6101) sports a bright X-ray trail and filament. The synchrotron emission from both structures is expected to be polarized, with electric vector position angle (EVPA) perpendicular to the magnetic field direction and polarization degree (PD) indicating the local degree of magnetic turbulence. We present a 1 […]


Continue.. IXPE Polarizations of the Lighthouse Pulsar, Trail, and Filament

Backlighting the Cosmic Web with Fast Radio Bursts: An Anthology of Dispersion Measure Cross-Correlations with Large-Scale Structure and Baryon Tracers

Kavli Affiliate: W. L. Kimmy Wu | Summary:Fast Radio Bursts (FRBs) probe baryons permeating the cosmic web through their dispersion measures (DMs), which encode the integrated electron density along cosmological sightlines. Using 3,455 unique FRB sources from CHIME/FRB with $sim 15$ arcmin localizations, we present an anthology of DM correlations with tracers of large-scale structure […]


Continue.. Backlighting the Cosmic Web with Fast Radio Bursts: An Anthology of Dispersion Measure Cross-Correlations with Large-Scale Structure and Baryon Tracers

The Effects of Complex Accretion Disk Geometry on Broadened Iron K$α$ Lines

Kavli Affiliate: Daniel R. Wilkins | Summary:X-rays are emitted from the corona above the orbiting matter of the accretion disk and travel either directly to us or illuminate the disk. This illumination of the inner disk is enhanced by gravitational light bending, which focuses the rays towards the black hole and therefore towards the inner […]


Continue.. The Effects of Complex Accretion Disk Geometry on Broadened Iron K$α$ Lines