Projected sensitivities of the LUX-ZEPLIN (LZ) experiment to new physics via low-energy electron recoils

Kavli Affiliate: T. A. Shutt | Summary:LUX-ZEPLIN (LZ) is a dark matter detector expected to obtain world-leading sensitivity to weakly interacting massive particles (WIMPs) interacting via nuclear recoils with a ~7-tonne xenon target mass. This manuscript presents sensitivity projections to several low-energy signals of the complementary electron recoil signal type: 1) an effective neutrino magnetic […]


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Constraints on Effective Field Theory Couplings Using 311.2 days of LUX Data

Kavli Affiliate: C. M. Ignarra | First 5 Authors: D. S. Akerib, S. Alsum, H. M. Araújo, X. Bai, J. Balajthy | Summary: We report here the results of an Effective Field Theory (EFT) WIMP search analysis using LUX data. We build upon previous LUX analyses by extending the search window to include nuclear recoil […]


Continue.. Constraints on Effective Field Theory Couplings Using 311.2 days of LUX Data

Constraints on Effective Field Theory Couplings Using 311.2 days of LUX Data

Kavli Affiliate: T. A. Shutt | Summary:We report here the results of an Effective Field Theory (EFT) WIMP search analysis using LUX data. We build upon previous LUX analyses by extending the search window to include nuclear recoil energies up to $sim$180 keV$_nr$, requiring a reassessment of data quality cuts and background models. In order […]


Continue.. Constraints on Effective Field Theory Couplings Using 311.2 days of LUX Data

Search for non-Newtonian interactions at micrometer scale with a levitated test mass

Kavli Affiliate: Giorgio Gratta | Summary:We report on a search for non-Newtonian forces that couple to mass, with a characteristic scale of $sim10~μ$m, using an optically levitated microsphere as a precision force sensor. A silica microsphere trapped in an upward-propagating, single-beam, optical tweezer is utilized to probe for interactions sourced from a nanofabricated attractor mass […]


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Breaking the degeneracy between polarization efficiency and cosmological parameters in CMB experiments

Kavli Affiliate: W. L. Kimmy Wu | First 5 Authors: Silvia Galli, W. L. Kimmy Wu, Karim Benabed, François Bouchet, Thomas M. Crawford | Summary: Accurate cosmological parameter estimates using polarization data of the cosmic microwave background (CMB) put stringent requirements on map calibration, as highlighted in the recent results from the Planck satellite. In […]


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Opportunities for DOE National Laboratory-led QuantISED Experiments

Kavli Affiliate: Peter Graham | First 5 Authors: Pete Barry, Karl Berggren, A. Baha Balantekin, John Bollinger, Ray Bunker | Summary: A subset of QuantISED Sensor PIs met virtually on May 26, 2020 to discuss a response to a charge by the DOE Office of High Energy Physics. In this document, we summarize the QuantISED […]


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The cosmology dependence of galaxy clustering and lensing from a hybrid $N$-body-perturbation theory model

Kavli Affiliate: Risa H. Wechsler | First 5 Authors: Nickolas Kokron, Joseph DeRose, Shi-Fan Chen, Martin White, Risa H. Wechsler | Summary: We implement a model for the two-point statistics of biased tracers that combines dark matter dynamics from $N$-body simulations with an analytic Lagrangian bias expansion. Using Aemulus, a suite of $N$-body simulations built […]


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Hunting for Dark Matter and New Physics with GECCO

Kavli Affiliate: Sven C. Herrmann | First 5 Authors: Adam Coogan, Alexander Moiseev, Logan Morrison, Stefano Profumo, Matthew G. Baring | Summary: We outline the science opportunities in the areas of searches for dark matter and new physics offered by a proposed future MeV gamma-ray telescope, the Galactic Explorer with a Coded Aperture Mask Compton […]


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PSR J1810+1744: Companion Darkening and a Precise High Neutron Star Mass

Kavli Affiliate: Roger W. Romani | First 5 Authors: Roger W. Romani, D. Kandel, Alexei V. Filippenko, Thomas G. Brink, WeiKang Zheng | Summary: Keck-telescope spectrophotometry of the companion of PSR J1810+1744 shows a flat, but asymmetric light-curve maximum and a deep, narrow minimum. The maximum indicates strong gravity darkening near the L_1 point, along […]


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