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Showing 2016Show all

468 papers · 1 filter

gr-qc2016★ 5 cited

Geodesics dynamics in the Linet-Tian spacetime with Lambda>0

Irene Brito, M. F. A. Da Silva, Filipe C. Mena +1

We analyse the geodesics' dynamics in cylindrically symmetric vacuum spacetimes with Lambda>0 and compare it to the Lambda=0 and Lambda<0 cases. When Lambda>0 there are two singula…

astro-ph.SR2016★ 58 cited

Period spacings in red giants; III. Coupling factors of mixed modes

B. Mosser, C. Pinçon, K. Belkacem +2

The power of asteroseismology relies on the capability of global oscillations to infer the stellar structure. For evolved stars, we benefit from unique information directly carried…

astro-ph.SR2016★ 69 cited

A model for stealth coronal mass ejections

B. J. Lynch, S. Masson, Y. Li +4

Stealth coronal mass ejections (CMEs) are events in which there are almost no observable signatures of the CME eruption in the low corona but often a well-resolved slow flux rope C…

astro-ph.EP2016★ 46 cited

First scattered-light images of the gas-rich debris disk around 49 Ceti

É. Choquet, J. Milli, Z. Wahhaj +31

We present the first scattered-light images of the debris disk around 49 ceti, a ~40 Myr A1 main sequence star at 59 pc, famous for hosting two massive dust belts as well as large…

astro-ph.GA2016★ 29 cited

In and out star formation in z~1.5 quiescent galaxies from rest-frame UV spectroscopy and the far-infrared

Raphael Gobat, Emanuele Daddi, Veronica Strazzullo +18

We present a sample of 34 spectroscopically confirmed BzK-selected ~1e11 Msun quiescent galaxies (pBzK) in the COSMOS field. The targets were initially observed with VIMOS on the V…

hep-ex2016★ 66 cited

Measurement of the CKM angle from a combination of LHCb results

LHCb collaboration, R. Aaij, B. Adeva +765

A combination of measurements sensitive to the CKM angle from LHCb is performed. The inputs are from analyses of time-integrated , $B^{0} \rightarrow D K…

astro-ph.EP2016★ 30 cited

Chromium isotope evidence in ejecta deposits for the nature of Paleoproterozoic impactors

Berengere Mougel, Frederic Moynier, Christa Gopel +1

Non-mass dependent chromium isotopic signatures have been successfully used to determine the presence and identification of extra-terrestrial materials in terrestrial impact rocks.…

astro-ph.HE2016★ 20 cited

Dark jets in the soft X-ray state of black hole binaries?

S. Drappeau, J. Malzac, M. Coriat +10

X-ray binary observations led to the interpretation that powerful compact jets, produced in the hard state, are quenched when the source transitions to its soft state. The aim of t…

astro-ph.HE2016★ 66 cited

The NuSTAR Serendipitous Survey: The 40 month Catalog and the Properties of the Distant High Energy X-ray Source Population

G. B. Lansbury, D. Stern, J. Aird +35

We present the first full catalog and science results for the NuSTAR serendipitous survey. The catalog incorporates data taken during the first 40 months of NuSTAR operation, which…

astro-ph.IM2016★ 7 cited

Dealing with missing data in the MICROSCOPE space mission: An adaptation of inpainting to handle colored-noise data

Sandrine Pires, Joel Bergé, Quentin Baghi +2

The MICROSCOPE space mission, launched on April 25, 2016, aims to test the weak equivalence principle (WEP) with a 10^-15 precision. To reach this performance requires an accurate…

gr-qc2016★ 4 cited

Semi-classical analysis of black holes in Loop Quantum Gravity: Modelling Hawking radiation with volume fluctuations

Pierre Heidmann, Hongguang Liu, Karim Noui

We introduce the notion of fluid approximation of a quantum spherical black hole in the context of Loop Quantum Gravity. In this limit, the microstates of the black hole are intert…

nucl-th2016

Holographic Photon Production and Anisotropic Flow

Ioannis Iatrakis, Elias Kiritsis, Chun Shen +1

The thermal-photon emission from strongly coupled gauge theories at finite temperature via the bottom-up models in holographic QCD in the deconfined phase is studied. The models ar…

math.AP2016★ 21 cited

Universality of blow up profile for small blow up solutions to the energy critical wave map equation

Thomas Duyckaerts, Hao Jia, Carlos Kenig +1

In this paper we introduce the channel of energy argument to the study of energy critical wave maps into the sphere. More precisely, we prove a channel of energy type inequality fo…

hep-th2016★ 11 cited

A Note on Vectorial AdS/CFT Duality for Spin- Boundary Theory

Jin-Beom Bae, Euihun Joung, Shailesh Lal

The vectorial holographic correspondences between higher-spin theories in AdS and free vector models on the boundary are extended to the cases where the latter is described by…

astro-ph.SR2016★ 21 cited

Period spacing of gravity modes strongly affected by rotation. Going beyond the traditional approximation

Vincent Prat, Stéphane Mathis, François Lignières +2

Context. As of today, asteroseismology mainly allows us to probe the internal rotation of stars when modes are only weakly affected by rotation using perturbative methods. Such met…

math.RT2016★ 1 cited

Sur une variante des troncatures d'Arthur

Pierre-Henri Chaudouard

We show that, for a large class of test functions, the unipotent contributions in the trace formula for over a number field, can be obtained from zeta functions and integra…

astro-ph.SR2016★ 13 cited

A Distant Mirror: Solar Oscillations Observed on Neptune by the Kepler K2 Mission

P. Gaulme, J. F. Rowe, T. R. Bedding +24

Starting in December 2014, Kepler K2 observed Neptune continuously for 49 days at a 1-minute cadence. The goals consisted of studying its atmospheric dynamics (Simon et al. 2016),…

astro-ph.SR2016★ 88 cited

Constraining the efficiency of angular momentum transport with asteroseismology of red giants: the effect of stellar mass

P. Eggenberger, N. Lagarde, A. Miglio +12

Context: Constraints on the internal rotation of red giants are now available thanks to asteroseismic observations. Preliminary comparisons with rotating stellar models indicate th…

astro-ph.GA2016★ 26 cited

Globular Clusters As Tracers of Fine Structure in the Dramatic Shell Galaxy NGC 474

Sungsoon Lim, Eric W. Peng, Pierre-Alain Duc +7

Globular clusters (GCs) are some of the most visible tracers of the merging and accretion history of galaxy halos. Metal-poor GCs, in particular, are thought to arrive in massive g…

cond-mat.str-el2016★ 4 cited

Raman Active High Energy Excitations in URuSi

Jonathan Buhot, Yann Gallais, Maximilien Cazayous +5

We have performed Raman scattering measurements on URuSi single crystals on a large energy range up to 1300 cm and in all the Raman active symmetries as a fun…

astro-ph.EP2016★ 111 cited

3D Radiation Non-ideal Magnetohydrodynamical Simulations Of The Inner Rim In Protoplanetary Disks

M. Flock, S. Fromang, N. J. Turner +1

Many planets orbit within an AU of their stars, raising questions about their origins. Particularly puzzling are the planets found near the silicate sublimation front. We investiga…

astro-ph.CO2016★ 49 cited

Cosmological constraints with weak lensing peak counts and second-order statistics in a large-field survey

Austin Peel, Chieh-An Lin, Francois Lanusse +3

Peak statistics in weak lensing maps access the non-Gaussian information contained in the large-scale distribution of matter in the Universe. They are therefore a promising complem…

astro-ph.SR2016★ 23 cited

Halpha Doppler shifts in a tornado in the solar corona

B. Schmieder, P. Mein, N. Mein +3

High resolution movies in 193 A from the Atmospheric Imaging Assembly (AIA) on the Solar Dynamic Observatory SDO show apparent rotation in the leg of a prominence observed during a…

astro-ph.GA2016★ 32 cited

Dense gas in low-metallicity galaxies

J. Braine, Y. Shimajiri, P. André +4

Stars form out of the densest parts of molecular clouds. Far-IR emission can be used to estimate the Star Formation Rate (SFR) and high dipole moment molecules, typically HCN, trac…