Author
James Battat
Other affiliations: Massachusetts Institute of Technology, Bryn Mawr College, Harvard University
Bio: James Battat is an academic researcher from Wellesley College. The author has contributed to research in topics: Dark matter & Detector. The author has an hindex of 26, co-authored 84 publications receiving 2433 citations. Previous affiliations of James Battat include Massachusetts Institute of Technology & Bryn Mawr College.
Topics: Dark matter, Detector, Physics, Time projection chamber, WIMP
Papers published on a yearly basis
Papers
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TL;DR: The white paper summarizes the workshop "U.S. Cosmic Visions: New Ideas in Dark Matter" held at University of Maryland on March 23-25, 2017.
Abstract: This white paper summarizes the workshop "U.S. Cosmic Visions: New Ideas in Dark Matter" held at University of Maryland on March 23-25, 2017.
464 citations
Boston University1, Perimeter Institute for Theoretical Physics2, University of Waterloo3, Massachusetts Institute of Technology4, Joseph Fourier University5, University of California, Los Angeles6, Occidental College7, University of Pennsylvania8, University of Zaragoza9, University of Sheffield10, Brandeis University11, Harvard University12, Nagasaki Institute of Applied Science13, University of Edinburgh14, University of New Mexico15, University of Huelva16, University of Utah17, University of Nottingham18, Kyoto University19, Lawrence Berkeley National Laboratory20, Temple University21, University of Warwick22, New York University23, Nagoya University24, University of Tokyo25, Saga University26, University of Ioannina27
TL;DR: The case for a dark matter detector with directional sensitivity was presented at the 2009 CYGNUS workshop on directional dark matter detection, and contributions from theorists and experimental groups in the field as mentioned in this paper.
Abstract: We present the case for a dark matter detector with directional sensitivity. This document was developed at the 2009 CYGNUS workshop on directional dark matter detection, and contains contributions from theorists and experimental groups in the field. We describe the need for a dark matter detector with directional sensitivity; each directional dark matter experiment presents their project's status; and we close with a feasibility study for scaling up to a one ton directional detector, which would cost around $150M.
224 citations
University of Grenoble1, University of Nottingham2, Wellesley College3, University of Lyon4, University of Amsterdam5, University of California, Los Angeles6, University of Utah7, Université Paris-Saclay8, University of Paris9, Princeton University10, Broad Institute11, University of New Mexico12, Royal Holloway, University of London13, University of Warwick14, Ohio State University15, University of Hawaii16
TL;DR: In this article, the authors review the potential of directional detectors for detecting and characterizing WIMPs and present a powerful tool for demonstrating the Galactic origin of nuclear recoils and hence unambiguously detecting Dark Matter.
209 citations
TL;DR: The Apache Point Observatory Lunar Laser-ranging Operation (APOLLO) has achieved 1m m range precision to the moon, which should lead to ap- proximately 1 order-of-magnitude improvements in several tests of fundamental properties of gravity.
Abstract: A next-generation lunar laser-ranging apparatus using the 35 m telescope at the Apache Point Observatory in southern New Mexico has begun science operation The Apache Point Observatory Lunar Laser-ranging Operation (APOLLO) has achieved 1m mrange precision to the moon, which should lead to ap- proximately 1 order-of-magnitude improvements in several tests of fundamental properties of gravity We briefly outline the scientific goals, and then give a detailed discussion of the APOLLO instrumentation
119 citations
TL;DR: This work constitutes the first LLR constraints on SME parameters, and finds no evidence for Lorentz violation at the 10(-6) to 10(-11) level in these parameters.
Abstract: We present constraints on violations of Lorentz invariance based on archival lunar laser-ranging (LLR) data. LLR measures the Earth-Moon separation by timing the round-trip travel of light between the two bodies and is currently accurate to the equivalent of a few centimeters (parts in ${10}^{11}$ of the total distance). By analyzing this LLR data under the standard-model extension (SME) framework, we derived six observational constraints on dimensionless SME parameters that describe potential Lorentz violation. We found no evidence for Lorentz violation at the ${10}^{\ensuremath{-}6}$ to ${10}^{\ensuremath{-}11}$ level in these parameters. This work constitutes the first LLR constraints on SME parameters.
107 citations
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TL;DR: There is, I think, something ethereal about i —the square root of minus one, which seems an odd beast at that time—an intruder hovering on the edge of reality.
Abstract: There is, I think, something ethereal about i —the square root of minus one. I remember first hearing about it at school. It seemed an odd beast at that time—an intruder hovering on the edge of reality.
Usually familiarity dulls this sense of the bizarre, but in the case of i it was the reverse: over the years the sense of its surreal nature intensified. It seemed that it was impossible to write mathematics that described the real world in …
33,785 citations
TL;DR: Tests of general relativity at the post-Newtonian level have reached high precision, including the light deflection, the Shapiro time delay, the perihelion advance of Mercury, the Nordtvedt effect in lunar motion, and frame-dragging.
Abstract: The status of experimental tests of general relativity and of theoretical frameworks for analyzing them is reviewed and updated. Einstein’s equivalence principle (EEP) is well supported by experiments such as the Eotvos experiment, tests of local Lorentz invariance and clock experiments. Ongoing tests of EEP and of the inverse square law are searching for new interactions arising from unification or quantum gravity. Tests of general relativity at the post-Newtonian level have reached high precision, including the light deflection, the Shapiro time delay, the perihelion advance of Mercury, the Nordtvedt effect in lunar motion, and frame-dragging. Gravitational wave damping has been detected in an amount that agrees with general relativity to better than half a percent using the Hulse-Taylor binary pulsar, and a growing family of other binary pulsar systems is yielding new tests, especially of strong-field effects. Current and future tests of relativity will center on strong gravity and gravitational waves.
3,394 citations
TL;DR: The Cologne Database for Molecular Spectroscopy (CDMS) as discussed by the authors contains a catalog of transition frequencies from the radio-frequency to the far-infrared region covering atomic and molecular species that (may) occur in the interstellar or circumstellar medium or in planetary atmospheres.
1,842 citations
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TL;DR: DESI as discussed by the authors is a ground-based dark energy experiment that will study baryon acoustic oscillations (BAO) and the growth of structure through redshift-space distortions with a wide-area galaxy and quasar redshift survey.
Abstract: DESI (Dark Energy Spectroscopic Instrument) is a Stage IV ground-based dark energy experiment that will study baryon acoustic oscillations (BAO) and the growth of structure through redshift-space distortions with a wide-area galaxy and quasar redshift survey. To trace the underlying dark matter distribution, spectroscopic targets will be selected in four classes from imaging data. We will measure luminous red galaxies up to $z=1.0$. To probe the Universe out to even higher redshift, DESI will target bright [O II] emission line galaxies up to $z=1.7$. Quasars will be targeted both as direct tracers of the underlying dark matter distribution and, at higher redshifts ($ 2.1 < z < 3.5$), for the Ly-$\alpha$ forest absorption features in their spectra, which will be used to trace the distribution of neutral hydrogen. When moonlight prevents efficient observations of the faint targets of the baseline survey, DESI will conduct a magnitude-limited Bright Galaxy Survey comprising approximately 10 million galaxies with a median $z\approx 0.2$. In total, more than 30 million galaxy and quasar redshifts will be obtained to measure the BAO feature and determine the matter power spectrum, including redshift space distortions.
965 citations