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200 papers

The absolute atomic mass of $^{208}$Pb has been determined with a fractional uncertainty of $7\times 10^{-11}$ by measuring the cyclotron-frequency ratio $R$ of $^{208}$Pb$^{41+}$ to $^{132}$Xe$^{26+}$ with the high-precision Penning-trap…

Evidence for the existence of a superheavy nucleus with atomic mass number A=292 and abundance (1-10)x10^(-12) relative to 232Th has been found in a study of natural Th using inductively coupled plasma-sector field mass spectrometry. The…

Nuclear Experiment · Physics 2011-04-07 A. Marinov , I. Rodushkin , D. Kolb , A. Pape , Y. Kashiv , R. Brandt , R. V. Gentry , H. W. Miller

We present intermediate resolution long-slit spectra and narrow-band Halpha, [NII] and [OIII] images of PM1-242, PM318 and PM1-333, three IRAS sources classified as possible planetary nebulae. The spectra show that the three objects are…

Astrophysics of Galaxies · Physics 2009-11-13 L. F. Miranda , C. B. Pereira , M. A. Guerrero

A gauge invariant, non-local observable is constructed in pure gauge theory, which is identical to the gluon propagator in a particular gauge, permitting to define a non-perturbative parton mass for the gluon. This mass can be shown to be…

High Energy Physics - Lattice · Physics 2007-05-23 O. Philipsen

The IceCube detector, which is embedded in the glacial ice at the geographic South Pole, is the first neutrino telescope to comprise a volume of one cubic kilometer. The search for neutrinos of astrophysical origin is among the primary…

High Energy Astrophysical Phenomena · Physics 2019-08-13 A. Franckowiak

Sensitive radio continuum surveys of the Galactic plane are ideal for discovering new supernova remnants (SNRs). From the Sino-German {\lambda}6 cm polarisation survey of the Galactic plane, an extended shell-like structure has been found…

Astrophysics of Galaxies · Physics 2020-03-11 X. Y. Gao , P. Reich , W. Reich , L. G. Hou , J. L. Han

Thanks to the use of advanced analysis techniques, the H.E.S.S. imaging Cherenkov telescope array has now reached a sensitivity level allowing the detection of sources with fluxes around 1% of the Crab with a limited observation time (less…

High Energy Astrophysical Phenomena · Physics 2019-08-14 Hélène Laffon , Fabio Acero , Francois Brun , Bruno Khélifi , Gerd Pühlhofer , Régis Terrier

The electron energy spectra, not connected to b-decay, of 235U- and 239Pu-films, irradiated by thermal neutrons, obtained by a Monte Carlo method is presented in the given work. The modelling was performed with the help of a computer code…

Nuclear Theory · Physics 2007-05-23 V. D. Rusova , V. N. Pavlovychb , V. A. Tarasova , S. V. Iaroshenkob , D. A. Litvinova

The possibility of existence of hyperons in the recently measured $2M_\odot$ pulsar PSRJ1614-2230 is explored using a diverse set of nuclear equations of state calculated within the relativistic mean-field models. Our results indicate that…

Nuclear Theory · Physics 2015-06-11 A. Sulaksono , B. K. Agrawal

The best measurement of the cosmic ray positron flux available today was performed by the HEAT balloon experiment more than 10 years ago. Given the limitations in weight and power consumption for balloon experiments, a novel approach was…

Astrophysics · Physics 2008-11-26 P. von Doetinchem , H. Gast , T. Kirn , G. Roper Yearwood , S. Schael

The deployment of a low-noise 3 kg p-type point contact germanium detector at the Dresden-II power reactor, 8 meters from its 2.96 GW$_{th}$ core, is described. This location provides an unprecedented (anti)neutrino flux of 8.1$\times…

High Energy Physics - Experiment · Physics 2021-10-13 J. Colaresi , J. I. Collar , T. W. Hossbach , A. R. L. Kavner , C. M. Lewis , A. E. Robinson , K. M. Yocum

Recent observations have led to the discovery of numerous optically selected binaries containing an undetected component with mass consistent with a compact object (neutron star or white dwarf). Using the the Neil Gehrels Swift Observatory…

High Energy Astrophysical Phenomena · Physics 2024-06-26 B. Sbarufatti , F. Coti Zelati , A. Marino , S. Mereghetti , N. Rea , A. Treves

As photodisintegration of deuterons mimics the disintegration of deuterons by neutrinos, the accurate measurement of the radioactivity from thorium and uranium decay chains in the heavy water in the Sudbury Neutrino Observatory (SNO) is…

Nuclear Experiment · Physics 2009-11-07 T. C. Andersen , SNO Collaboration

We present Herschel PACS photometry of 18 Plutinos and determine sizes and albedos for these objects using thermal modeling. We analyze our results for correlations, draw conclusions on the Plutino size distribution, and compare to earlier…

The IceCube Neutrino Observatory at the South Pole has been completed in December 2010. In this paper we describe the final detector and report results on physics and performance using data taken at different stages of the yet incomplete…

High Energy Astrophysical Phenomena · Physics 2012-08-27 The IceCube Collaboration

We searched for the appearance of pi+pi- pairs with invariant mass greater than 648 MeV in a neutral beam. Such an observation could signify the decay of a long-lived light neutral particle. We find no evidence for this decay. Our null…

High Energy Physics - Experiment · Physics 2008-11-26 J. Adams

The neutron gyromagnetic ratio has been measured relative to that of the 199Hg atom with an uncertainty of 0.8 ppm. We employed an apparatus where ultracold neutrons and mercury atoms are stored in the same volume and report the result…

We report the first mass measurement of the proton-halo candidate $^{22}$Al performed with the LEBIT facility's 9.4~T Penning trap mass spectrometer at FRIB. This measurement completes the mass information for the lightest remaining…

New measurements to test the neutrality of matter by acoustic means are reported. The apparatus is based on a spherical capacitor filled with gaseous SF$_6$ excited by an oscillating electric field. The apparatus has been calibrated…

Atomic Physics · Physics 2015-05-27 G. Bressi , G. Carugno , F. Della Valle , G. Galeazzi , G. Ruoso , G. Sartori

The archival spectrum of SDSSJ212531.92-010745.9 shows not only the typical signature of a PG1159 star, but also indicates the presence of a companion. Our aim was the proof of the binary nature ofthis object and the determination of its…