Electromagnetic probes of primordial black holes as dark matter

Kavli Affiliate: A. C. Davis | First 5 Authors: Y. Ali-Haimoud, S. Clesse, J. Garcia-Bellido, A. Kashlinsky, L. Wyrzykowski | Summary: The LIGO discoveries have rekindled suggestions that primordial black holes (BHs) may constitute part to all of the dark matter (DM) in the Universe. Such suggestions came from 1) the observed merger rate of […]


Continue.. Electromagnetic probes of primordial black holes as dark matter

Constraining the Tail-End of Reionization Using Lyman-$α$ Transmission Spikes

Kavli Affiliate: Nickolay Gnedin | First 5 Authors: Enrico Garaldi, Nickolay Gnedin, Piero Madau, , | Summary: We investigate Lyman-$alpha$ transmission spikes at $z > 5$ in synthetic quasar spectra, and discuss their connection to the properties of the intergalactic medium and their ability to constrain reionization models. We use state-of-the-art radiation-hydrodynamic simulations from the […]


Continue.. Constraining the Tail-End of Reionization Using Lyman-$α$ Transmission Spikes

Research and Development for Near Detector Systems Towards Long Term Evolution of Ultra-precise Long-baseline Neutrino Experiments

Kavli Affiliate: Mark Hartz | First 5 Authors: Aysel Kayis Topaksu, Edward Blucher, Bernard Andrieu, Jianming Bian, Byron Roe | Summary: With the discovery of non-zero value of $theta_{13}$ mixing angle, the next generation of long-baseline neutrino (LBN) experiments offers the possibility of obtaining statistically significant samples of muon and electron neutrinos and anti-neutrinos with […]


Continue.. Research and Development for Near Detector Systems Towards Long Term Evolution of Ultra-precise Long-baseline Neutrino Experiments

The ultra-diffuse galaxy NGC 1052-DF2 with MUSE: I. Kinematics of the stellar body

Kavli Affiliate: Eric Peng | First 5 Authors: Eric Emsellem, Remco F. J. van der Burg, Jeremy Fensch, Tereza Jerabkova, Anita Zanella | Summary: The so-called ultra-diffuse galaxy NGC~1052-DF2 was announced to be a galaxy lacking dark matter based on a spectroscopic study of its constituent globular clusters. Here we present the first spectroscopic analysis […]


Continue.. The ultra-diffuse galaxy NGC 1052-DF2 with MUSE: I. Kinematics of the stellar body

Future Opportunities in Accelerator-based Neutrino Physics

Kavli Affiliate: Masayuki Nakahata | First 5 Authors: Andrea Dell’Acqua, Antoni Aduszkiewicz, Markus Ahlers, Hiroaki Aihara, Tyler Alion | Summary: This document summarizes the conclusions of the Neutrino Town Meeting held at CERN in October 2018 to review the neutrino field at large with the aim of defining a strategy for accelerator-based neutrino physics in […]


Continue.. Future Opportunities in Accelerator-based Neutrino Physics

Future Opportunities in Accelerator-based Neutrino Physics

Kavli Affiliate: Masayuki Nakahata | First 5 Authors: Andrea Dell’Acqua, Antoni Aduszkiewicz, Markus Ahlers, Hiroaki Aihara, Tyler Alion | Summary: This document summarizes the conclusions of the Neutrino Town Meeting held at CERN in October 2018 to review the neutrino field at large with the aim of defining a strategy for accelerator-based neutrino physics in […]


Continue.. Future Opportunities in Accelerator-based Neutrino Physics

Ground motion prediction at gravitational wave observatories using archival seismic data

Kavli Affiliate: Richard Mittleman | First 5 Authors: Nikhil Mukund, Michael Coughlin, Jan Harms, Sebastien Biscans, Jim Warner | Summary: Gravitational wave observatories have always been affected by tele-seismic earthquakes leading to a decrease in duty cycle and coincident observation time. In this analysis, we leverage the power of machine learning algorithms and archival seismic […]


Continue.. Ground motion prediction at gravitational wave observatories using archival seismic data

Candidate Massive Galaxies at $z sim 4$ in the Dark Energy Survey

Kavli Affiliate: Rafe Schindler | First 5 Authors: Pierandrea Guarnieri, Claudia Maraston, Daniel Thomas, Janine Pforr, Violeta Gonzalez-Perez | Summary: Using stellar population models, we predicted that the Dark Energy Survey (DES) – due to its special combination of area (5000 deg. sq.) and depth ($i = 24.3$) – would be in the position to […]


Continue.. Candidate Massive Galaxies at $z sim 4$ in the Dark Energy Survey