activity
20062023
most citedThe Atacama Cosmology Telescope: Cosmological parameters from three seasons of data

350 citations · 4.4k across the 76 of their papers we have counts for

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Showing 2019Show all

7 papers · 1 filter

hep-ph2019★ 40 cited

Prospects for Detecting Boosted Dark Matter in DUNE through Hadronic Interactions

Joshua Berger, Yanou Cui, Mathew Graham +5

Boosted dark matter (BDM) is a well-motivated class of dark matter (DM) candidates in which a small component of DM is relativistic at the present time. We lay the foundation for B…

hep-ph2019★ 63 cited

Ultralight dark matter detection with mechanical quantum sensors

Daniel Carney, Anson Hook, Zhen Liu +2

We consider the use of quantum-limited mechanical force sensors to detect ultralight (sub-meV) dark matter candidates which are weakly coupled to the standard model. We show that m…

astro-ph.HE2019★ 7 cited

Soft excess in the quiescent Be/X-ray pulsar RX J0812.4-3114

Yue Zhao, Craig O. Heinke, Sergey S. Tsygankov +3

We report a 72 ks XMM-Newton observation of the Be/X-ray pulsar (BeXRP) RX J0812.4-3114 in quiescence (). Intriguingly, we find…

hep-ph2019★ 67 cited

Searching for Dark Photon Dark Matter in LIGO O1 Data

Huai-Ke Guo, Keith Riles, Feng-Wei Yang +1

Dark matter exists in our Universe, but its nature remains mysterious. The remarkable sensitivity of the Laser Interferometer Gravitational-Wave Observatory (LIGO) may be able to s…

hep-ph2019★ 130 cited

Probing Axions with Event Horizon Telescope Polarimetric Measurements

Yifan Chen, Jing Shu, Xiao Xue +2

With high spatial resolution, polarimetric imaging of a supermassive black hole, like M87 or Sgr A, by the Event Horizon Telescope can be used to probe the existenc…

astro-ph.CO2019★ 50 cited

Detecting Axion-like Dark Matter with Linearly Polarized Pulsar Light

Tao Liu, George Smoot, Yue Zhao

Non-relativistic QCD axions or axion-like particles are among the most popular candidates for cold Dark Matter (DM) in the universe. We proposed to detect axion-like DM, using line…