Khachatryan, V Sirunyan, AM Tumasyan, A Adam, W Bergauer, T Dragicevic, M Eroe, J Fabjan, C Friedl, M Fruehwirth, R
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Searches for supersymmetry (SUSY) are presented based on the electroweak pair production of neutralinos and charginos, leading to decay channels with Higgs, Z, and W bosons and undetected lightest SUSY particles (LSPs). The data sample corresponds to an integrated luminosity of about 19.5 fb−1 of proton-proton collisions at a center-of-mass energy ...
Gainsforth, Z Westphal, AJ Butterworth, AL Jilly-Rehak, CE Brownlee, DE Joswiak, D Ogliore, RC Zolensky, ME Bechtel, HA Ebel, DS
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In a consortium analysis of a large particle captured from the coma of comet 81P/Wild 2 by the Stardust spacecraft, we report the discovery of a field of fine-grained material (FGM) in contact with a large sulfide particle. The FGM was partially located in an embayment in the sulfide. As a consequence, some of the FGM appears to have been protected...
Van Roestel, J Groot, PJ Kupfer, T Verbeek, K Van Velzen, S Bours, M Nugent, P Prince, T Levitan, D Nissanke, S
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© 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. We present results of the Sky2Night project: a systematic, unbiased search for fast optical transients with the Palomar Transient Factory. We have observed 407deg 2 in R-band for eight nights at a cadence of 2 h. During the entire duration of the ...
Lepaulard, C Gattacceca, J Swanson-Hysell, N Quesnel, Y Demory, F Osinski, GR
© The Meteoritical Society, 2019. We report paleomagnetic directions from the target rocks of the Tunnunik impact structure, as well as from lithic impact breccia dikes that formed during the impact event. The target sedimentary rocks have been remagnetized after impact-related tilting during a reverse polarity interval. Their magnetization is unbl...
Jenniskens, P Utas, J Yin, QZ Matson, RD Fries, M Howell, JA Free, D Albers, J Devillepoix, H Bland, P
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© The Meteoritical Society, 2019. It has been proposed that all L chondrites resulted from an ongoing collisional cascade of fragments that originated from the formation of the ~500 Ma old asteroid family Gefion, located near the 5:2 mean-motion resonance with Jupiter in the middle Main Belt. If so, L chondrite pre-atmospheric orbits should be dist...
Korre, L Garaud, P Brummell, NH
We study the dynamics associated with the extension of turbulent convective motions from a convection zone (CZ) into a stable region (RZ) that lies below the latter. For that purpose, we have run a series of three-dimensional direct numerical simulations solving the Navier-Stokes equations under the Boussinesq approximation in a spherical shell geo...
Mackenroth, F Bulanov, SS
© 2019 Author(s). Ion beams generated with ultra-intense laser-plasma accelerators hold promises to provide compact and affordable beams of relativistic ions. One of the most efficient acceleration setups was demonstrated to be direct acceleration by the laser's radiation pressure. Due to plasma instabilities developing in the ultra-thin foils requ...
Graham, ML Harris, CE Nugent, PE Maguire, K Sullivan, M Smith, M Valenti, S Goobar, A Fox, OD Shen, KJ
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© 2019. The American Astronomical Society. All rights reserved. The nature and role of the binary companion of carbon-oxygen white dwarf stars that explode as Type Ia supernovae (SNe Ia) are not yet fully understood. Past detections of circumstellar material (CSM) that contain hydrogen for a small number of SN Ia progenitor systems suggest that at ...
Brush, M Linder, EV Zumalacárregui, M
© 2019 IOP Publishing Ltd and Sissa Medialab. No Slip Gravity is a simple modified gravity theory with only one free function and the interesting characteristic that - unlike many modified gravity theories - it suppresses growth. This allows it to fit current redshift space distortion and σ 8 mass fluctuation amplitude data better than ΛCDM in gene...
Yoon, M James Jee, M Anthony Tyson, J Schmidt, S Wittman, D Choi, A
© 2019. The American Astronomical Society. All rights reserved.. We present cosmological parameter measurements from the Deep Lens Survey (DLS) using galaxy-mass and galaxy-galaxy power spectra in the multipole range ℓ = 250-2000. We measure galaxy-galaxy power spectra from two lens bins centered at z ∼ 0.27 and 0.54 and galaxy-mass power spectra b...