papers

Publications (13)

astro-ph.CO2016

Using the Crab Nebula as a high precision calibrator for Cosmic Microwave Background polarimeters

Jonathan Kaufman, Brian Keating, David Leon

The polarization of the Cosmic Microwave Background (CMB) provides a plethora of information about the early universe. Most notably, gravitational waves from the Inflationary epoch…

quant-ph2018

Cosmic Bell Test using Random Measurement Settings from High-Redshift Quasars

Dominik Rauch, Johannes Handsteiner, Armin Hochrainer +17

In this Letter, we present a cosmic Bell experiment with polarization-entangled photons, in which measurement settings were determined based on real-time measurements of the wavele…

astro-ph.IM2017

Performance of a continuously rotating half-wave plate on the POLARBEAR telescope

Satoru Takakura, Mario Aguilar, Yoshiki Akiba +50

A continuously rotating half-wave plate (CRHWP) is a promising tool to improve the sensitivity to large angular scales in cosmic microwave background (CMB) polarization measurement…

astro-ph.HE2020

Improved Constraints on Anisotropic Birefringent Lorentz Invariance and CPT Violation from Broadband Optical Polarimetry of High Redshift Galaxies

Andrew S. Friedman, Roman Gerasimov, Fabian Kislat +4

In the framework of the Standard Model Extension (SME), we present improved constraints on anisotropic Lorentz invariance and Charge-Parity-Time (CPT) violation by searching for as…

astro-ph.CO2016

POLARBEAR Constraints on Cosmic Birefringence and Primordial Magnetic Fields

POLARBEAR Collaboration, Peter A. R. Ade, Kam Arnold +84

We constrain anisotropic cosmic birefringence using four-point correlations of even-parity -mode and odd-parity -mode polarization in the cosmic microwave background measurem…

astro-ph.CO2019

Constraints on Scalar and Tensor spectra from

Ido Ben-Dayan, Brian Keating, David Leon +1

At the linear level, the gravitational wave (GW) spectrum predicted by inflation, and many of its alternatives, can have arbitrarily small amplitude and consequently an unconstrain…

astro-ph.CO2020

Measurement of the Cosmic Microwave Background Polarization Lensing Power Spectrum from Two Years of POLARBEAR Data

Mario Aguilar Faúndez, Kam Arnold, Carlo Baccigalupi +48

We present a measurement of the gravitational lensing deflection power spectrum reconstructed with two seasons cosmic microwave background polarization data from the POLARBEAR expe…

astro-ph.HE2018

Constraints on Lorentz Invariance and CPT Violation using Optical Photometry and Polarimetry of Active Galaxies BL Lacertae and S5 B0716+714

Andrew S. Friedman, David Leon, Kevin D. Crowley +5

Various quantum gravity approaches that extend beyond the standard model predict Lorentz Invariance and Charge-Parity-Time Violation at energies approaching the Planck scale. These…

astro-ph.IM2016

Making maps of Cosmic Microwave Background polarization for B-mode studies: the POLARBEAR example

Davide Poletti, Giulio Fabbian, Maude Le Jeune +46

Analysis of cosmic microwave background (CMB) datasets typically requires some filtering of the raw time-ordered data. Filtering is frequently used to minimize the impact of low fr…

astro-ph.HE2019

Standard-Model Extension Constraints on Lorentz and CPT Violation From Optical Polarimetry of Active Galactic Nuclei

Andrew S. Friedman, David Leon, Roman Gerasimov +9

Vacuum birefringence from Lorentz and CPT violation in the Standard-Model Extension can be constrained using ground-based optical polarimetry of extragalactic sources. We describe…

astro-ph.CO2019

Evidence for the Cross-correlation between Cosmic Microwave Background Polarization Lensing from POLARBEAR and Cosmic Shear from Subaru Hyper Suprime-Cam

Toshiya Namikawa, Yuji Chinone, Hironao Miyatake +72

We present the first measurement of cross-correlation between the lensing potential, reconstructed from cosmic microwave background (CMB) {\it polarization} data, and the cosmic sh…

astro-ph.CO2019

The Simons Observatory: Science goals and forecasts

The Simons Observatory Collaboration, Peter Ade, James Aguirre +247

The Simons Observatory (SO) is a new cosmic microwave background experiment being built on Cerro Toco in Chile, due to begin observations in the early 2020s. We describe the scient…

astro-ph.CO2016

The Cosmic Microwave Background And Pseudo-Nambu-Goldstone Bosons: Searching For Lorentz Violations In The Cosmos

David Leon, Jonathan Kaufman, Brian Keating +1

One of the most powerful probes of new physics is the polarized Cosmic Microwave Background (CMB). The detection of a nonzero polarization angle rotation between the CMB surface of…