output
20022025
most citedObservation of a new particle in the search for the Standard Model Higgs boson with the ATLAS detector at the LHC

10.9k citations

Showing 2013Show all

26 papers · 1 filter

nucl-th2013

Nuclear state densities of odd-mass heavy nuclei in the shell model Monte Carlo approach

C. Özen, Y. Alhassid, H. Nakada

While the shell model Monte Carlo approach has been successful in the microscopic calculation of nuclear state densities, it has been difficult to calculate accurately state densit…

astro-ph.EP2013255 cited

Kepler-62: A five-planet system with planets of 1.4 and 1.6 Earth radii in the Habitable Zone

W. J. Borucki, E. Agol, F. Fressin +62

We present the detection of five planets -- Kepler-62b, c, d, e, and f -- of size 1.31, 0.54, 1.95, 1.61 and 1.41 Earth radii, orbiting a K2V star at periods of 5.7, 12.4, 18.2, 12…

math.OA2013

Spectral gap actions and invariant states

Han Li, Chi-Keung Ng

We define spectral gap actions of discrete groups on von Neumann algebras and study their relations with invariant states. We will show that a finitely generated ICC group is i…

cs.DB2013

Learning and Verifying Quantified Boolean Queries by Example

Azza Abouzied, Dana Angluin, Christos Papadimitriou +2

To help a user specify and verify quantified queries --- a class of database queries known to be very challenging for all but the most expert users --- one can question the user on…

q-bio.NC2013

Synaptic Scaling Balances Learning in a Spiking Model of Neocortex

Mark Rowan, Samuel Neymotin

Learning in the brain requires complementary mechanisms: potentiation and activity-dependent homeostatic scaling. We introduce synaptic scaling to a biologically-realistic spiking…

astro-ph.SR201348 cited

Characterizing the Cool KOIs. V. KOI-256: A Mutually Eclipsing Post-Common Envelope Binary

Philip S. Muirhead, Andrew Vanderburg, Avi Shporer +23

We report that Kepler Object of Interest 256 (KOI-256) is a mutually eclipsing post-common envelope binary (ePCEB), consisting of a cool white dwarf (M = 0.592 +/- 0.089 MSun, R =…