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20072026
most citedConstraining Dark Matter-Baryon Scattering with Linear Cosmology

306 citations · 2.5k across the 57 of their papers we have counts for

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13 papers · 1 filter

astro-ph.CO2026

Gravitational lensing time delay beyond the Shapiro/geometry split

Luca Teodori, Kfir Blum, Zhaoyu Bai

Time delays are a key observable in strong gravitational lensing systems. Their theoretical expression is usually written as a sum of a geometrical delay and a Shapiro delay, with…

astro-ph.CO2025★ 8 cited

Bracketing the soliton-halo relation of ultralight dark matter

Kfir Blum, Marco Gorghetto, Edward Hardy +1

In theories of ultralight dark matter, solitons form in the inner regions of galactic halos. The observational implications of these depend on the soliton mass. Various relations b…

astro-ph.CO2024

AxionH0graphy: hunting for ultralight dark matter with cosmographic H signal

Kfir Blum, Luca Teodori

If ultralight boson fields exist, then vacuum misalignment populates them with nonzero relic abundance. For a broad range of particle mass the field condenses into fuzzy cores…

astro-ph.CO2023★ 4 cited

Host group degeneracy in gravitational lensing time delay determination of

Luca Teodori, Kfir Blum

Massive elliptical galaxies, that serve as lenses in gravitational lensing time delay measurements of the Hubble parameter , often reside in a host group. We consider degenera…

astro-ph.CO2022

Comments on the mass sheet degeneracy in cosmography analyses

Luca Teodori, Kfir Blum, Emanuele Castorina +2

We make a number of comments regarding modeling degeneracies in strong lensing measurements of the Hubble parameter . The first point concerns the impact of weak lensing assoc…

astro-ph.CO2021★ 25 cited

Gravitational lensing tension from ultralight axion galactic cores

Kfir Blum, Luca Teodori

Gravitational lensing time delays offer an avenue to measure the Hubble parameter , with some analyses suggesting a tension with early-type probes of . The lensing measur…

astro-ph.CO2020★ 65 cited

Could quasar lensing time delays hint to a core component in halos, instead of H0 tension?

Kfir Blum, Emanuele Castorina, Marko Simonović

The time delay measured between the images of gravitationally lensed quasars probes a combination of the angular diameter distance to the source-lens system and the mass density pr…

astro-ph.CO2019★ 87 cited

Looking for ultralight dark matter near supermassive black holes

Nitsan Bar, Kfir Blum, Thomas Lacroix +1

Measurements of the dynamical environment of supermassive black holes (SMBHs) are becoming abundant and precise. We use such measurements to look for ultralight dark matter (ULDM),…

astro-ph.CO2019★ 81 cited

Ultra-light dark matter in disk galaxies

Nitsan Bar, Kfir Blum, Joshua Eby +1

Analytic arguments and numerical simulations show that bosonic ultra-light dark matter (ULDM) would form cored density distributions (`solitons') at the center of galaxies. ULDM so…

astro-ph.CO2018★ 192 cited

Galactic Rotation Curves vs. Ultra-Light Dark Matter: Implications of the Soliton -- Host Halo Relation

Nitsan Bar, Diego Blas, Kfir Blum +1

Bosonic ultra-light dark matter (ULDM) would form cored density distributions at the center of galaxies. These cores, seen in numerical simulations, admit analytic description as t…

astro-ph.CO2016★ 75 cited

CMB constraints on primordial black hole dark matter

Daniel Aloni, Kfir Blum, Raphael Flauger

We revisit cosmic microwave background (CMB) constraints on primordial black hole dark matter. Spectral distortion limits from COBE/FIRAS do not impose a relevant constraint. Planc…

astro-ph.CO2013★ 306 cited

Constraining Dark Matter-Baryon Scattering with Linear Cosmology

Cora Dvorkin, Kfir Blum, Marc Kamionkowski

We derive constraints on elastic scattering between baryons and dark matter using the cosmic microwave background (CMB) data from the Planck satellite and the Lyman-alpha forest da…

astro-ph.CO2013★ 19 cited

Perturbed Recombination from Dark Matter Annihilation

Cora Dvorkin, Kfir Blum, Matias Zaldarriaga

We show that dark matter annihilation around the time of recombination can lead to growing ionization fraction perturbations, that track the linear collapse of matter over-densitie…