Faster CMB lensing with control variates

Kavli Affiliate: Blake Sherwin | Summary:We present a new method for fast computation of the realization-dependent bias, a major computational bottleneck in measurements of the cosmic microwave background (CMB) lensing power spectrum. The method accelerates the bias calculation by differencing two correlated estimates: one based on fully realistic masked simulations and the other on isotropic […]


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SDSS-V: Revealing a weak accretion state in X-ray selected red quasars

Kavli Affiliate: Claudio Ricci | Summary:Red quasars (rQSOs) have been recognized as a short-lived, early stage in the evolutionary cycle of Active Galactic Nuclei (AGN), with fundamental differences in their intrinsic properties compared to blue quasars (bQSOs). In this work, we present the first large X-ray sample of 380 rQSOs, selected from the eROSITA/SDSS-V collaboration, […]


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A Wafer-Scale Heterogeneous III-V-on-Silicon Nitride Quantum Photonic Platform

Kavli Affiliate: Nergis Mavalvala | Summary:Heterogeneous integration of gain and strongly nonlinear materials with ultra-low-loss silicon nitride (SiN) photonics offers a route to scalable quantum circuits, but concurrent wafer-scale manufacturability, low interlayer loss, and high performance have been challenging to realize. Here we demonstrate a wafer-scale III-V-on-SiN quantum photonic platform that directly integrates III-V layers […]


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Chemical Interpretation of Time-Dependent Coupled-Cluster Theory

Kavli Affiliate: Thomas Crawford | Summary:While providing a highly accurate framework for simulating laser-induced many-electron dynamics in atom and molecules, including linear and nonlinear steady-state and transient absorption spectra, time-dependent coupled-cluster theory does not offer a straightforward interpretation in chemical terms. This should be contrasted with conventional time-independent equation-of-motion coupled-cluster or frequency-dependent response models where […]


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High-Frequency Thermal Noise in Michelson Interferometers

Kavli Affiliate: Lee McCuller | Summary:New experiments are being developed without the background of quantum shot noise to look for weak, high-frequency signals using Michelson interferometers. Since shot noise is no longer the dominant noise source with these readout schemes, it is important to accurately model thermal noise to characterize signals and design more sensitive […]


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Bidirectional Internal Squeezing for Gravitational-Wave Detectors

Kavli Affiliate: Lee McCuller | Summary:We present a bidirectional internal squeezing scheme for gravitational-wave detectors and show that it saturates the lowest known lower bounds on quantum noise from internal optical dissipation. The scheme uses two optical parametric amplification stages inside the signal-extraction cavity that act on intra-cavity fields propagating in opposite directions. Thereby, most […]


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Analytical method for computing the covariance matrix of cosmic shear two-point correlation function

Kavli Affiliate: Masahiro Takada | Summary:Accurate estimation of the covariance matrix of cosmic shear statistics is essential for cosmological analyses using current and upcoming wide-area weak lensing surveys. In this work, we investigate analytical methods for computing the Gaussian covariance matrix of the cosmic shear two-point correlation function (2PCF), taking into account the effects of […]


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Clusters Hiding Under Millimeter Sources (CHUMS) I: Extreme CHUMS

Kavli Affiliate: Adam Mantz | Summary:Galaxy cluster abundance provides a powerful probe of the $Λ$CDM model and enables precise constraints on cosmological parameters. Millimeter-wavelength surveys detect clusters through the Sunyaev-Zeldovich (SZ) effect, and are particularly effective at high redshifts. However, the SZ signal can be significantly contaminated by emission from Active Galactic Nuclei (AGN), particularly […]


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Warm, not Fuzzy: Generalized Ultralight Dark Matter Limits from Milky Way Satellites

Kavli Affiliate: Risa Wechsler | Summary:We generalize lower limits on the dark matter (DM) particle mass $m$ derived from Milky Way (MW) satellite galaxy abundances to scenarios in which DM is an ultralight scalar field produced with a field power spectrum peaked at a subhorizon wavenumber $k_*$. In these models, the DM field free-streams similar […]


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Correlation Between X-Ray and Cosmic Neutrino Sources: From Obscured AGN to Blazars

Kavli Affiliate: Claudio Ricci | Summary:The origin of high-energy astrophysical neutrinos remains a key open question in multimessenger astrophysics. A correlation between unabsorbed hard X-ray emission and high-energy neutrino luminosity has been reported in a sample of six active galactic nuclei with the highest individual IceCube significances, linking neutrino production to compact, photon-rich environments near […]


Continue.. Correlation Between X-Ray and Cosmic Neutrino Sources: From Obscured AGN to Blazars