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The $\nuebar$ flux and spectrum have been measured at a distance of about 800 m from the reactors of the Palo Verde Nuclear Generating Station using a segmented Gd-loaded liquid scintillator detector. Correlated positron-neutron events from…

High Energy Physics - Experiment · Physics 2019-08-17 F. Boehm , J. Busenitz , B. Cook , G. Gratta , H. Henrikson , J. Kornis , D. Lawrence , K. B. Lee , K. McKinny , L. Miller , V. Novikov , A. Piepke , B. Ritchie , D. Tracy , P. Vogel , Y-F. Wang , J. Wolf

The sterile neutrino interpretation of the LSND and MiniBooNE neutrino anomalies is currently being tested at three Liquid Argon detectors: MicroBooNE, SBND, and ICARUS. It has been argued that a degeneracy between $\nu_\mu \to \nu_e$ and…

High Energy Physics - Phenomenology · Physics 2025-03-19 Ohana Benevides Rodrigues , Matheus Hostert , Kevin J. Kelly , Bryce Littlejohn , Pedro A. N. Machado , Ibrahim Safa , Tao Zhou

We combine emission line and X-ray luminosities for 45 sources from the Chandra Deep Field South (CDF-S), and seven HELLAS sources, to obtain a new sample of 52 X-ray selected type-II active galactic nuclei (AGNs). Eighteen of our sources…

Astrophysics · Physics 2009-11-11 Hagai Netzer , V. Mainieri , P. Rosati , Benny Trakhtenbrot

We report Coulomb drag measurements on GaAs-AlGaAs electron-hole bilayers. The two layers are separated by a 10 or 25nm barrier. Below T$\approx$1K we find two features that a Fermi-liquid picture cannot explain. First, the drag on the hole…

Mesoscale and Nanoscale Physics · Physics 2009-10-27 A. F. Croxall , K. Das Gupta , C. A. Nicoll , M. Thangaraj , H. E. Beere , I. Farrer , D. A. Ritchie , M. Pepper

The Gamma Ray Imaging Spectrometer (GRIS) recently observed the gamma-ray emission from the Galactic center region. We have detected the 1809 keV Galactic 26Al emission at a significance level of 6.8-sigma but have found no evidence for…

We discuss the diffuse flux of electron neutrinos and antineutrinos from cosmological failed supernovae, stars that collapse directly into a black hole, with no explosion. This flux has a hotter energy spectrum compared to regular,…

Cosmology and Nongalactic Astrophysics · Physics 2015-03-17 James G. Keehn , Cecilia Lunardini

Recent experimental results in $B$ physics from Belle, BaBar and LHCb suggest new physics (NP) in the weak $b\to c$ charged-current and the $b\to s$ neutral-current processes. Here we focus on the charged-current case and specifically on…

High Energy Physics - Phenomenology · Physics 2023-01-18 Bhubanjyoti Bhattacharya , Thomas E. Browder , Quinn Campagna , Alakabha Datta , Shawn Dubey , Lopamudra Mukherjee , Alexei Sibidanov

In this work, a search for nuclearites of strange quark matter by using nine years of ANTARES data taken in the period 2009-2017 is presented. The passage through matter of these particles is simulated %according to the model of de…

High Energy Astrophysical Phenomena · Physics 2024-09-02 ANTARES Collaboration , A. Albert , S. Alves , M. André , M. Ardid , S. Ardid , J. -J. Aubert , J. Aublin , B. Baret , S. Basa , B. Belhorma , M. Bendahman , F. Benfenati , V. Bertin , S. Biagi , M. Bissinger , J. Boumaaza , M. Bouta , M. C. Bouwhuis , H. Brânzaş , R. Bruijn , J. Brunner , J. Busto , B. Caiffi , D. Calvo , A. Capone , L. Caramete , J. Carr , V. Carretero , S. Celli , M. Chabab , T. N. Chau , R. Cherkaoui El Moursli , T. Chiarusi , M. Circella , J. A. B. Coelho , A. Coleiro , R. Coniglione , P. Coyle , A. Creusot , A. F. Díaz , G. de Wasseige , B. De Martino , C. Distefano , I. Di Palma , A. Domi , C. Donzaud , D. Dornic , D. Drouhin , T. Eberl , T. van Eeden , D. van Eijk , N. El Khayati , A. Enzenhöfer , P. Fermani , G. Ferrara , F. Filippini , L. Fusco , J. García , P. Gay , H. Glotin , R. Gozzini , R. Gracia Ruiz , K. Graf , C. Guidi , S. Hallmann , H. van Haren , A. J. Heijboer , Y. Hello , J. J. Hernández-Rey , J. Hößl , J. Hofestädt , F. Huang , G. Illuminati , C. W. James , B. Jisse-Jung , M. de Jong , P. de Jong , M. Kadler , O. Kalekin , U. Katz , A. Kouchner , I. Kreykenbohm , V. Kulikovskiy , R. Lahmann , M. Lamoureux , R. Le Breton , D. Lefèvre , E. Leonora , G. Levi , S. Le Stum , D. Lopez-Coto , S. Loucatos , L. Maderer , J. Manczak , M. Marcelin , A. Margiotta , A. Marinelli , J. A. Martínez-Mora , K. Melis , P. Migliozzi , A. Moussa , R. Muller , L. Nauta , S. Navas , E. Nezri , B. Ó Fearraigh , A. Păun , G. E. Păvălaş , C. Pellegrino , M. Perrin-Terrin , V. Pestel , P. Piattelli , C. Pieterse , C. Poirè , V. Popa , T. Pradier , N. Randazzo , D. Real , S. Reck , G. Riccobene , A. Romanov , A. Sánchez-Losa , F. Salesa Greus , D. F. E. Samtleben , M. Sanguineti , P. Sapienza , J. Schnabel , J. Schumann , F. Schüssler , J. Seneca , M. Spurio , Th. Stolarczyk , M. Taiuti , Y. Tayalati , S. J. Tingay , B. Vallage , V. Van Elewyck , F. Versari , S. Viola , D. Vivolo , J. Wilms , S. Zavatarelli , A. Zegarelli , J. D. Zornoza , J. Zúñiga

SDSS J015957.64+003310.5 is an X-ray selected, $z=0.31$ AGN from the Stripe 82X survey that transitioned from a Type 1 quasar to a Type 1.9 AGN between 2000 and 2010. This is the most distant AGN, and first quasar, yet observed to have…

Both the recent 2009 and 2020 solar minima were classified as unusually quiet and characterized with unusually high galactic cosmic ray (GCR) levels. However, unlike the trends from previous decades in which anomalous cosmic ray (ACR) and…

Solar and Stellar Astrophysics · Physics 2023-02-22 R. D. Strauss , R. A. Leske , J. S. Rankin

We propose a novel approach for studying $\nu_\mu \to \nu_\tau$ oscillations with extragalactic neutrinos. Active Galactic Nuclei and Gamma Ray Bursts are believed to be sources of ultrahigh energy muon neutrinos. With distances of 100 Mpc…

High Energy Physics - Phenomenology · Physics 2010-12-03 Sharada Iyer , Mary Hall Reno , Ina Sarcevic

Branching fraction measurements from Fourier transform spectra in conjunction with published radiative lifetimes are used to determine transition probabilities for 263 lines of neutral chromium. These laboratory values are employed to…

Astrophysics · Physics 2009-11-13 Jennifer S. Sobeck , James E. Lawler , Christopher Sneden

We report the serendipitous detection by GALEX of fast (<1 day) rising (>1 mag) UV emission from two Type II plateau (II-P) supernovae (SNe) at z=0.185 and 0.324 discovered by the Supernova Legacy Survey. Optical photometry and VLT…

Gamma-ray lines from cosmic sources provide unique isotopic information, since they originate from energy level transitions in the atomic nucleus. Gamma-ray telescopes explored this astronomical window in the past three decades, detecting…

Astrophysics · Physics 2009-11-10 Roland Diehl , Nikos Prantzos , Peter von Ballmoos

The recent coincident detection of gravitational waves (GW) from a binary neutron star merger with aLIGO/Virgo and short-lived gamma-ray emission with Fermi/GBM (called GW 170817) is a milestone for the establishment of multi-messenger…

High Energy Astrophysical Phenomena · Physics 2017-10-17 J. Michael Burgess , Jochen Greiner , Damien Begue , Dimitrios Giannios , Francesco Berlato , Vladimir M. Lipunov

Experiments showing a seasonal variation of the nuclear decay rates of a number of different nuclei, and decay anomalies apparently related to solar flares and solar rotation, have suggested that the Sun may somehow be influencing nuclear…

Solar and Stellar Astrophysics · Physics 2015-06-05 D. E. Krause , B. A. Rogers , E. Fischbach , J. B Buncher , A. Ging , J. H. Jenkins , J. M. Longuski , N. Strange , P. A. Sturrock

In 2011, a re-evaluation of the antineutrino spectrum emitted by nuclear reactors revealed a 6% deficit between the observed flux and the expected one. This anomaly is significant at 2.9$\sigma$ and can be explained by a new oscillation at…

Instrumentation and Detectors · Physics 2016-02-02 Stéphane Zsoldos

Electron capture (EC) decay relies on attachment and stripping cross-sections, that in turn, depend on the atomic number of the nucleus. We revisit the impact of EC decay in the context of the high-precision cosmic-ray fluxes measured by…

High Energy Astrophysical Phenomena · Physics 2023-09-25 M. Borchiellini , D. Maurin , M. Vecchi