activity
20162022
most citedGalactic Rotation Curves vs. Ultra-Light Dark Matter: Implications of the Soliton -- Host Halo Relation

192 citations · 660 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.GA2022★ 14 cited

Dynamical friction in globular cluster-rich ultra-diffuse galaxies: the case of NGC5846-UDG1

Nitsan Bar, Shany Danieli, Kfir Blum

Ultra-diffuse galaxies that contain a large sample of globular clusters (GCs) offer an opportunity to test the predictions of galactic dynamics theory. NGC5846-UDG1 is an excellent…

hep-ph2021★ 73 cited

Galactic rotation curves versus ultralight dark matter: A systematic comparison with SPARC data

Nitsan Bar, Kfir Blum, Chen Sun

We look for and place observational constraints on the imprint of ultralight dark matter (ULDM) soliton cores in rotation-dominated galaxies. Extending previous analyses, we find a…

astro-ph.GA2021★ 28 cited

Assessing the Fornax globular cluster timing problem in different models of dark matter

Nitsan Bar, Diego Blas, Kfir Blum +1

We investigate what the orbits of globular clusters (GCs) in the Fornax dwarf spheroidal (dSph) galaxy can teach us about dark matter (DM). This problem was recently studied for ul…

hep-ph2019★ 165 cited

Is there a supernova bound on axions?

Nitsan Bar, Kfir Blum, Guido D'Amico

We present a critical assessment of the SN1987A supernova cooling bound on axions and other light particles. Core-collapse simulations used in the literature to substantiate the bo…

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.HE2018★ 4 cited

Neutrino flavour as a test of the explosion mechanism of core-collapse supernovae

Nitsan Bar, Kfir Blum, Guido D'Amico

We study the ratio of neutrino-proton elastic scattering to inverse beta decay event counts, measurable in a scintillation detector like JUNO, as a key observable for identifying t…

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…

physics.flu-dyn2016★ 16 cited

Turbulent thermal diffusion in strongly stratified turbulence: theory and experiments

G. Amir, N. Bar, A. Eidelman +3

Turbulent thermal diffusion is a combined effect of the temperature stratified turbulence and inertia of small particles. It causes the appearance of a non-diffusive turbulent flux…