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

980 citations

Showing 2015Show all

17 papers · 1 filter

nucl-th2015★ 5 cited

Electromagnetic form factors of one neutron halos with spin 1/2+ ground state

Lakma Fernando, Akshay Vaghani, Gautam Rupak

The electromagnetic form factors for single neutron halo nuclei Be-11, C-15 and C-19 are calculated. The calculations are performed in halo effective field theory (EFT) where the h…

astro-ph.CO2015

Uniformity of Cosmic Microwave Background as a Non-Inflationary Geometrical Effect

Branislav Vlahovic, Maxim Eingorn, Cosmin Ilie

The conventional CDM cosmological model supplemented by the inflation concept describes the Universe very well. However, there are still a few concerns: new Planck data impose c…

physics.ins-det2015★ 26 cited

The COHERENT Experiment at the Spallation Neutron Source

COHERENT Collaboration, D. Akimov, P. An +64

The COHERENT collaboration's primary objective is to measure coherent elastic neutrino-nucleus scattering (CEvNS) using the unique, high-quality source of tens-of-MeV neutrinos pro…

gr-qc2015★ 14 cited

Perfect fluids with as sources of scalar cosmological perturbations

Maxim Eingorn, Ruslan Brilenkov

We make a generalization of a self-consistent first-order perturbation scheme, being suitable for all (sub-horizon and super-horizon) scales, which has been recently constructed fo…

gr-qc2015★ 58 cited

First-order Cosmological Perturbations Engendered by Point-like Masses

Maxim Eingorn

In the framework of the concordance cosmological model the first-order scalar and vector perturbations of the homogeneous background are derived in the weak gravitational field lim…

hep-ex2015★ 38 cited

Search for double-beta decay of 136Xe to excited states of 136Ba with the KamLAND-Zen experiment

Zen Collaboration, K. Asakura, A. Gando +42

A search for double-beta decays of 136Xe to excited states of 136Ba has been performed with the first phase data set of the KamLAND-Zen experiment. The 0+1, 2+1 and 2+2 transitions…