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S. Tiwari

40 papers hereh-index 5522.1k citations154 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author2
  • middle author26
  • last author7

Across the 35 of 40 papers where every author was matched, so the position is known.

fields
  • gr-qc31
  • astro-ph.GA3
  • astro-ph.HE3
  • astro-ph.CO1
  • hep-th1
  • math.DG1
same name
  • S. Tiwari — 70 papers, h 25
  • S. Tiwari — 22 papers, h 19
  • S. Tiwari — 13 papers, h 15
  • S. Tiwari — 12 papers, h 7
  • S. Tiwari — 10 papers, h 61
  • S. Tiwari — 9 papers, h 6

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20152026
most citedMethod for detection and reconstruction of gravitational wave transients with networks of advanced detectors

465 citations · 1.8k across the 39 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

3 papers · 1 filter

astro-ph.HE2022

Prospects for detecting and localizing short-duration transient gravitational waves from glitching neutron stars without electromagnetic counterparts

Dixeena Lopez, Shubhanshu Tiwari, Marco Drago +3

Neutron stars are known to show accelerated spin-up of their rotational frequency called a glitch. Highly magnetized rotating neutron stars (pulsars) are frequently observed by rad…

astro-ph.HE2020★ 31 cited

Observing an intermediate mass black hole GW190521 with minimal assumptions

Marek Szczepanczyk, Sergey Klimenko, Brendan O'Brien +10

On May 21, 2019 Advanced LIGO and Advanced Virgo detectors observed a gravitational-wave transient GW190521, the heaviest binary black-hole merger detected to date with the remnant…

astro-ph.HE2019★ 149 cited

All-sky search for continuous gravitational waves from isolated neutron stars using Advanced LIGO O2 data

The LIGO Scientific Collaboration, the Virgo Collaboration, B. P. Abbott +1130

We present results of an all-sky search for continuous gravitational waves (CWs), which can be produced by fast-spinning neutron stars with an asymmetry around their rotation axis,…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.