output
19972026
most citedSearch for Majorana Neutrinos near the Inverted Mass Hierarchy Region with KamLAND-Zen

980 citations

Showing 2013Show all

22 papers · 1 filter

astro-ph.SR2013★ 6 cited

Exoplanetary searches with gravitational microlensing: polarization issues

A. F. Zakharov, G. Ingrosso, F. De Paolis +4

There are different methods for finding exoplanets such as radial spectral shifts, astrometrical measurements, transits, timing etc. Gravitational microlensing (including pixel-len…

physics.ins-det2013★ 11 cited

CeLAND: search for a 4th light neutrino state with a 3 PBq 144Ce-144Pr electron antineutrino generator in KamLAND

A. Gando, Y. Gando, S. Hayashida +63

The reactor neutrino and gallium anomalies can be tested with a 3-4 PBq (75-100 kCi scale) 144Ce-144Pr antineutrino beta-source deployed at the center or next to a large low-backgr…

astro-ph.GA2013★ 85 cited

Constraining the range of Yukawa gravity interaction from S2 star orbits

D. Borka, P. Jovanović, V. Borka Jovanović +1

We consider possible signatures for Yukawa gravity within the Galactic Central Parsec, based on our analysis of the S2 star orbital precession around the massive compact dark objec…

gr-qc2013★ 9 cited

Kaluza-Klein multidimensional models with Ricci-flat internal spaces: the absence of the KK particles

Alexey Chopovsky, Maxim Eingorn, Alexander Zhuk

In this paper we consider a multidimensional Kaluza-Klein (KK) model with a Ricci-flat internal space, e.g., a Calabi-Yau manifold. We perturb this background metrics by a system o…

hep-ph2013★ 154 cited

Dark Sectors and New, Light, Weakly-Coupled Particles

R. Essig, J. A. Jaros, W. Wester +86

Dark sectors, consisting of new, light, weakly-coupled particles that do not interact with the known strong, weak, or electromagnetic forces, are a particularly compelling possibil…

astro-ph.SR2013★ 12 cited

Polarization in binary microlensing events

G. Ingrosso, F. De Paolis, A. A. Nucita +5

The light received by source stars in microlensing events may be significantly polarized if both an efficient photon scattering mechanism is active in the source stellar atmosphere…