activity
20182021
most citedUltra-light dark matter in disk galaxies

81 citations · 81 across the 1 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2021

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

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

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.CO201981 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

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

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…