output
19932026
most citedMeasurements of Omega and Lambda from 42 High-Redshift Supernovae

18.1k citations

Showing 2017Show all

181 papers · 1 filter

physics.atom-ph2017★ 1 cited

Emergence of Spatial Order in Highly Interacting Rydberg Gases

João D. Rodrigues, Hugo Terças, Luis F. Gonçalves +2

We describe the emergence of strong spatial correlations, akin to liquid-like behavior and crystallization effects, in low (one and two) dimensional gases of cold Rydberg atoms. Th…

astro-ph.GA2017★ 13 cited

The ESO's VLT Type Ia supernova spectral set of the final two years of SNLS

C. Balland, F. Cellier-Holzem, C. Lidman +24

We aim to present 70 spectra of 68 new high-redshift type Ia supernovae (SNeIa) measured at ESO's VLT during the final two years of operation (2006-2008) of the Supernova Legacy Su…

cond-mat.mes-hall2017★ 22 cited

Valley polarized magnetic state in hole-doped mono layers of transition metal dichalcogenides

João E. H. Braz, B. Amorim, Eduardo V. Castro

We compute the valley/magnetic phase diagram of mono layers of transition metal dichalcogenides in the hole doped region where spin-orbit effects are particularly relevant. Taking…

cond-mat.mes-hall2017★ 21 cited

Link between the photonic and electronic topological phases in artificial graphene

Sylvain Lannebère, Mário G. Silveirinha

In recent years the study of topological phases of matter has emerged as a very exciting field of research, both in photonics and in electronics. However, up to now the electronic…

astro-ph.HE2017★ 41 cited

Studying the Ultraviolet Spectrum of the First Spectroscopically Confirmed Supernova at redshift two

M. Smith, M. Sullivan, R. C. Nichol +87

We present observations of DES16C2nm, the first spectroscopically confirmed hydrogen-free superluminous supernova (SLSN-I) at redshift z~2. DES16C2nm was discovered by the Dark Ene…

gr-qc2017★ 10 cited

Black hole horizons can hide positive heat capacity

Tamás S. Biró, Viktor G. Czinner, Hideo Iguchi +1

Regarding the volume as independent thermodynamic variable we point out that black hole horizons can hide positive heat capacity and specific heat. Such horizons are mechanically m…

cond-mat.mes-hall2017★ 23 cited

Impact of complex adatom-induced interactions on quantum spin Hall phases

Flaviano Jose dos Santos, Dario A. Bahamon, Roberto B. Muniz +4

Adsorbate engineering offers a seemingly simple approach to tailor spin-orbit interactions in atomically thin materials and thus to unlock the much sought-after topological insulat…

physics.ins-det2017★ 13 cited

MARTA: A high-energy cosmic-ray detector concept with high-accuracy muon measurement

P. Abreu, S. Andringa, P. Assis +42

A new concept for the direct measurement of muons in air showers is presented. The concept is based on resistive plate chambers (RPCs), which can directly measure muons with very g…

gr-qc2017★ 84 cited

Spinning particles in general relativity: Momentum-velocity relation for the Mathisson-Pirani spin condition

L. Filipe O. Costa, Georgios Lukes-Gerakopoulos, Oldřich Semerák

The Mathisson-Papapetrou-Dixon (MPD) equations, providing the "pole-dipole" description of spinning test particles in general relativity, have to be supplemented by a condition spe…

gr-qc2017★ 9 cited

Rotating elastic string loops in flat and black hole spacetimes: stability, cosmic censorship and the Penrose process

Jose Natario, Leonel Queimada, Rodrigo Vicente

We rederive the equations of motion for relativistic strings, that is, one-dimensional elastic bodies whose internal energy depends only on their stretching, and use them to study…

hep-ph2017★ 4 cited

Lepton mixing and the charged-lepton mass ratios

D. Jurciukonis, L. Lavoura

We construct a class of renormalizable models for lepton mixing that generate predictions given in terms of the charged-lepton mass ratios. We show that one of those models leads,…

gr-qc2017★ 3 cited

Black hole mass formula in the membrane paradigm

José P. S. Lemos, Oleg B. Zaslavskii

The membrane paradigm approach adopts a timelike surface, stretched out off the null event horizon, to study several important black hole properties. We use this powerful tool to g…

gr-qc2017★ 479 cited

Dynamical systems applied to cosmology: dark energy and modified gravity

Sebastian Bahamonde, Christian G. Boehmer, Sante Carloni +3

The Nobel Prize winning confirmation in 1998 of the accelerated expansion of our Universe put into sharp focus the need of a consistent theoretical model to explain the origin of t…

hep-ph2017★ 37 cited

Fermion Masses and Mixings and Dark Matter Constraints in a Model with Radiative Seesaw Mechanism

Nicolás Bernal, A. E. Cárcamo Hernández, Ivo de Medeiros Varzielas +1

We formulate a predictive model of fermion masses and mixings based on a family symmetry. In the quark sector the model leads to the viable mixing inspired texture where th…

hep-ph2017★ 13 cited

Radiative neutrino masses from order-4 CP symmetry

Igor P. Ivanov

Generalized CP symmetry of order 4 (CP4) is surprisingly powerful in shaping scalar and quark sectors of multi-Higgs models. Here, we extend this framework to the neutrino sector.…

cond-mat.stat-mech2017★ 73 cited

Dynamical phase transitions at finite temperature from fidelity and interferometric Loschmidt echo induced metrics

Bruno Mera, Chrysoula Vlachou, Nikola Paunković +2

We study finite-temperature Dynamical Quantum Phase Transitions (DQPTs) by means of the fidelity and the interferometric Loschmidt Echo (LE) induced metrics. We analyse the associa…

gr-qc2017★ 20 cited

Solving the relativistic inverse stellar problem through gravitational waves observation of binary neutron stars

Tiziano Abdelsalhin, Andrea Maselli, Valeria Ferrari

The LIGO/Virgo collaboration has recently announced the direct detection of gravitational waves emitted in the coalescence of a neutron star binary. This discovery allows, for the…

cs.RO2017★ 38 cited

Language Bootstrapping: Learning Word Meanings From Perception-Action Association

Giampiero Salvi, Luis Montesano, Alexandre Bernardino +1

We address the problem of bootstrapping language acquisition for an artificial system similarly to what is observed in experiments with human infants. Our method works by associati…

hep-ph2017★ 63 cited

The C2HDM revisited

Duarte Fontes, Margarete Mühlleitner, Jorge C. Romão +3

The complex two-Higgs doublet model is one of the simplest ways to extend the scalar sector of the Standard Model to include a new source of CP-violation. The model has been used a…

hep-lat2017

Tetraquark resonances computed with static lattice QCD potentials and scattering theory

Pedro Bicudo, Marco Cardoso, Antje Peters +2

We study tetraquark resonances with lattice QCD potentials computed for two static quarks and two dynamical quarks, the Born-Oppenheimer approximation and the emergent wave method…

quant-ph2017★ 39 cited

Spontaneous lateral atomic recoil force close to a photonic topological material

S. Ali Hassani Gangaraj, George W. Hanson, Mauro Antezza +1

We investigate the quantum recoil force acting on an excited atom close to the surface of a nonreciprocal photonic topological insulator (PTI). The main atomic emission channel is…

hep-th2017★ 62 cited

Quasinormal modes of black holes in Einstein-power-Maxwell theory

Grigoris Panotopoulos, Angel Rincon

In the present work we compute the spectrum of quasinormal frequencies of four-dimensional charged black holes in Einstein-power-Maxwell theory. In particular we study scalar pertu…

astro-ph.HE2017★ 193 cited

Search for High-energy Neutrinos from Binary Neutron Star Merger GW170817 with ANTARES, IceCube, and the Pierre Auger Observatory

A. Albert, M. Andre, M. Anghinolfi +1931

The Advanced LIGO and Advanced Virgo observatories recently discovered gravitational waves from a binary neutron star inspiral. A short gamma-ray burst (GRB) that followed the merg…

quant-ph2017★ 11 cited

Quantum contract signing with entangled pairs

P. Yadav, P. Mateus, N. Paunković +1

We present a quantum scheme for signing contracts between two clients (Alice and Bob) using entangled states and the services of a third trusted party (Trent). The trusted party is…