works on

From the 2 of 3.3k papers with an AI index.

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19922026
most citedGW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

9.8k citations

3,257 papers

astro-ph.SR2026

Effects of radial conductivity variation on the Ponomarenko dynamo

Shipra Verma, Kannabiran Seshasayanan

We study the effects of conductivity variation on the Ponomarenko dynamo. Taking monotonically increasing/decreasing and sinusoidally varying radial profiles, we study the kinemati…

astro-ph.HE2026

Large small-scale kinematic dynamo in protoneutron stars

Shipra Verma, Kannabiran Seshasayanan, Raphaël Raynaud +1

Magnetars are young, isolated neutron stars that possess an exceptionally strong magnetic field, with surface dipolar strengths on the order of G. One of the plausible sc…

physics.flu-dyn2026★ 7 cited

Sloshing reduction in a swaying tank with porous baffles using scaled boundary finite element method

Pramod, Aln, Choudhury +5

Sloshing is an inevitable phenomenon in an ocean-going vessel that can have adverse effects. In this work, the mitigation of sloshing is investigated using multiple thin porous baf…

eess.SY2026

A (Purely) Graph-Theoretic Approach to Synchronization of Nonlinear Dynamical Networks

Aandrew Baggio Sahaya Arokiadoss, G. Arunkumar

Synchronizing nonlinear dynamical networks typically requires solving matrix inequalities or detailed system models, which fail for large networks. This paper offers a simple fix :…

cs.CV2026★ 5 cited

SHFormer: Dynamic Spectral Filtering Convolutional Neural Network and High-pass Kernel Generation Transformer for Adaptive MRI Reconstruction

Sriprabha Ramanarayanan, Rahul G. S., Mohammad Al Fahim +3

Attention Mechanism (AM) selectively focuses on essential information for imaging tasks and captures relationships between distant pixel neighborhoods to compute feature representa…

astro-ph.CO2026

Observational Frontiers in the post-EoR 21-cm Intensity Mapping: Lessons from the SKA Pathfinders

Khandakar Md Asif Elahi, Somnath Bharadwaj, Philip Bull +21

The 21-cm line from neutral hydrogen has long been recognised as a promising tracer of the large-scale structure of the Universe. The line is weak however, making individual galaxy…