Publications by authors named "R Karuppusamy"

Magnetars-highly magnetized neutron stars-are thought to be the most likely progenitors for fast radio bursts (FRBs). Freely precessing magnetars are further invoked to explain the repeating FRBs. We report here on new high-cadence radio observations of the magnetar XTE J1810-197 recorded shortly after an X-ray outburst.

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Article Synopsis
  • Pulsar Timing Array experiments are used to investigate the existence of ultralight dark matter particles by observing an ensemble of millisecond radio pulsars over several years.
  • The second data release from the European Pulsar Timing Array focuses on a scenario where dark matter only interacts with regular matter through gravity.
  • The findings indicate that while ultralight dark matter particles in a specific mass range cannot make up all of the local dark matter density, they can exist at a maximum local density of around 0.3 GeV/cm³.
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Covid-19 is a multisystem disease with the lungs being predominantly affected. Cardiac involvement is mostly seen as a rise in troponins, arrhythmias, and ventricular dysfunction. This study aimed to estimate the incidence of arrhythmias seen in Covid-19 infection and assess if arrhythmias predict worsening or mortality Prospective observational study involving patients with mild to moderate Covid illness admitted in a tertiary care centre.

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Fast radio bursts (FRBs) are flashes of unknown physical origin. The majority of FRBs have been seen only once, although some are known to generate multiple flashes. Many models invoke magnetically powered neutron stars (magnetars) as the source of the emission.

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The 2017 Event Horizon Telescope (EHT) observations of the central source in M87 have led to the first measurement of the size of a black-hole shadow. This observation offers a new and clean gravitational test of the black-hole metric in the strong-field regime. We show analytically that spacetimes that deviate from the Kerr metric but satisfy weak-field tests can lead to large deviations in the predicted black-hole shadows that are inconsistent with even the current EHT measurements.

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