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19922026
most citedNeutrino Masses and Leptogenesis with Heavy Higgs Triplets

518 citations

Showing 2019Show all

105 papers · 1 filter

hep-ph2019

Exploring Dark Matter, Neutrino mass and flavour anomalies in L_μ-L_τ model

Rukmani Mohanta, Shivaramakrishna Singirala, Suchismita Sahoo

We investigate Majorana dark matter in a new variant of gauge extension of Standard Model, containing three additional neutral fermions , along wi…

hep-ph2019★ 6 cited

On Resolving the Dark LMA Solution at Neutrino Oscillation Experiments

Sandhya Choubey, Dipyaman Pramanik

In presence of non standard interactions, the solar neutrino data is consistent with two solutions, one close to the standard LMA solution with and anothe…

cond-mat.str-el2019

A theory of resistivity in Kondo lattice materials: the memory function approach

Komal Kumari, Raman Sharma, Navinder Singh +1

We theoretically analyse D.C. resistivity() in the Kondo-lattice model using the powerful memory function approach. The complete temperature evolution of is investigated usi…

quant-ph2019★ 7 cited

Selective tuning of Hilbert spaces in states encoded with spatial modes of light

Ali Anwar, Nijil Lal, Shashi Prabhakar +1

Spatial modes of light directly give the most easily accessible degree of freedom that span an infinite dimensional Hilbert space. The higher dimensional spatial mode entanglement…

astro-ph.GA2019★ 16 cited

Unveiling the importance of magnetic fields in the evolution of dense clumps formed at the waist of bipolar H II regions: a case study on Sh2-201 with JCMT SCUBA-2/POL-2

Chakali Eswaraiah, Di Li, Manash R. Samal +10

We present the properties of magnetic fields (B-fields) in two clumps (clump 1 and clump 2), located at the waist of the bipolar H II region Sh2-201, based on JCMT SCUBA-2/POL-2 ob…

astro-ph.IM2019

Characterisation of Cosmic Ray Induced Noise Events in AstroSat-CZT Imager

Debdutta Paul, A. R. Rao, Ajay Ratheesh +6

The Cadmium Zinc Telluride (CZT) Imager onboard AstroSat, consists of pixelated CZT detectors, which are sensitive to hard X-rays above 20 keV. The individual pixels are triggered…

astro-ph.CO2019★ 49 cited

Primordial black holes and gravitational waves in nonstandard cosmologies

Sukannya Bhattacharya, Subhendra Mohanty, Priyank Parashari

For primordial black holes (PBHs) to form a considerable fraction of cold dark matter, the required amplitude of primordial scalar perturbations is quite large ($P_ζ(k) \sim 10^{-2…

astro-ph.SR2019★ 8 cited

A Hot Cusp-Shaped Confined Solar Flare

Aaron Hernandez-Perez, Yang Su, Julia K. Thalmann +5

We analyze a confined flare that developed a hot cusp-like structure high in the corona (H ~ 66 Mm). A growing cusp-shaped flare arcade is a typical feature in the standard model o…

astro-ph.GA2019★ 6 cited

New insights in giant molecular cloud hosting S147/S153 complex: signatures of interacting clouds

J. S. Dhanya, L. K. Dewangan, D. K. Ojha +1

In order to understand the formation of massive OB stars, we report a multi-wavelength observational study of a giant molecular cloud hosting the S147/S153 complex (size ~90 pc X 5…

cond-mat.quant-gas2019★ 1 cited

Quantum Hall states for in optical lattices

Rukmani Bai, Soumik Bandyopadhyay, Sukla Pal +2

We examine the quantum Hall (QH) states of the optical lattices with square geometry using Bose-Hubbard model (BHM) in presence of artificial gauge field. In particular, we focus o…

hep-ph2019★ 14 cited

Heavy quark transport in a viscous semi QGP

Balbeer Singh, Hiranmaya Mishra

We study the effect of shear and bulk viscosities on the heavy quark transport coefficient within the matrix model of semi QGP. Dissipative effects are incorporated through the fir…

astro-ph.SR2019★ 9 cited

A new tool for predicting the solar cycle: Correlation between flux transport at the equator and the poles

Susanta Kumar Bisoi, P. Janardhan

The magnetic flux cancellation on the Sun plays a crucial role in determining the manner in which the net magnetic flux changes in every solar cycle, affecting the large scale evol…

physics.atom-ph2019★ 31 cited

Analytic Response Relativistic Coupled-Cluster Theory: The first application to indium isotope shifts

B. K. Sahoo, A. R. Vernon, R. F. Garcia Ruiz +16

With increasing demand for accurate calculation of isotope shifts of atomic systems for fundamental and nuclear structure research, an analytic energy derivative approach is presen…

hep-ph2019★ 1 cited

Pure Natural Quintessential Inflation and Dark Energy

Selvaganapathy J

We propose the pure natural quintessential inflation model which is motivated by Witten's conjecture, where the axion couples to pure Yang-Mills gauge field at large N limi…

astro-ph.CO2019★ 19 cited

Inflation models in the light of self-interacting sterile neutrinos

Arindam Mazumdar, Subhendra Mohanty, Priyank Parashari

Short baseline neutrino experiments, like LSND and MiniBooNE experiments, pointed towards the existence of eV mass scale sterile neutrinos. To reconcile sterile neutrinos with cosm…

astro-ph.CO2019★ 6 cited

Magnetic fields in a hot dense neutrino plasma and the Gravitational Waves

Arun Kumar Pandey, Pravin Kumar Natwariya, Jitesh R Bhatt

In the present work, we have studied the spectrum of the primordial gravitational waves due to magnetic instability in the presence of neutrino asymmetry. The magnetic instability…

hep-ph2019★ 5 cited

Soft leptogenesis in the NMSSM with a singlet right-handed neutrino superfield

Waleed Abdallah, Abhass Kumar, Abhijit Kumar Saha

In this work, we explore soft leptogenesis in the NMSSM framework extended by a right-handed neutrino superfield. We calculate the CP asymmetry, , and find it to be no…

astro-ph.SR2019★ 3 cited

Infrared spectroscopy of the recent outburst in V1047 Cen (Nova Centauri 2005)

T. R. Geballe, D. P. K. Banerjee, A. Evans +14

Fourteen years after its eruption as a classical nova (CN), V1047 Cen (Nova Cen 2005) began an unusual re-brightening in 2019 April. The amplitude of the brightening suggests that…

astro-ph.IM2019★ 1 cited

Solar X-ray Monitor (XSM) On-board Chandrayaan-2 Orbiter

M. Shanmugam, S. V. Vadawale, Arpit R. Patel +17

Solar X-ray Monitor (XSM) is one of the scientific instruments on-board Chandrayaan-2 orbiter. The XSM along with instrument CLASS (Chandras Large Area Soft x-ray Spectrometer) com…

physics.atom-ph2019★ 5 cited

A Comparative Analysis of Non-relativistic and Relativistic Calculations of Electric Dipole Moments and Polarizabilities of Heteronuclear Alkali Dimers

R. Mitra, V. S. Prasannaa, B. K. Sahoo

We analyze the molecular electric dipole moments (PDMs) and static electric dipole polarizabilities of heteronuclear alkali dimers in their ground states by employing coupled-clust…

astro-ph.SR2019

Investigation of a confined C-class flare in an arch filament system close to a regular sunspot

Rohan Eugene Louis

A moderate C1.1 class confined flare is investigated here, which occurred on 2013 September 24 at 22:56~UT, in an arch filament system close to a regular, unipolar sunspot. Spectro…

astro-ph.CO2019★ 45 cited

Formation of Primordial Black Holes from Warm Inflation

Richa Arya

Primordial Black Holes (PBHs) serve as a unique probe to the physics of the early Universe, particularly inflation. In light of this, we study the formation of PBHs by the collapse…

astro-ph.SR2019★ 21 cited

Another Mini Solar Maximum in the Offing: A Prediction for the Amplitude of Solar Cycle 25

Susanta Kumar Bisoi, P. Janardhan, S. Ananthakrishnan

We examine the temporal changes in both solar polar magnetic field (PMF) at latitudes and heliospheric magnetic field (HMF) at 1 AU during solar cycles 21--24 wi…

astro-ph.HE2019★ 12 cited

NuSTAR view of Be/X-ray binary pulsar 2S 1417-624 during 2018 giant outburst

Shivangi Gupta, Sachindra Naik, Gaurava K. Jaisawal

We report the results obtained from a detailed timing and spectral studies of Be/X-ray binary pulsar 2S 1417-624 using data from Swift and NuSTAR observatories. The observations we…