◍wovepaper
SearchResearchersInstitutions
Sign in
researcher

S. Sharma

4 papers hereh-index 171.9k citations249 works total

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

author position
  • first author2
  • middle author2

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO3
  • physics.plasm-ph1
same name
  • S. Sharma — 382 papers
  • S. Sharma — 242 papers
  • S. Sharma — 88 papers
  • S. Sharma — 82 papers
  • S. Sharma — 74 papers
  • S. Sharma — 51 papers, h 18

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
20112021
most citedSpatiotemporal evolution of a self-excited dust density wave in a nanodusty plasma under strong Havnes effect

17 citations · 25 across the 4 of their papers we have counts for

collaborators

4 papers

physics.plasm-ph2021★ 17 cited

Spatiotemporal evolution of a self-excited dust density wave in a nanodusty plasma under strong Havnes effect

Bidyut Chutia, T. Deka, Y. Bailung +3

A broad-spectrum self-excited dust density wave is experimentally studied in a vertically extended nanodusty plasma consisting of in situ grown carbonaceous nanometer sized particl…

astro-ph.CO2013

Electric and Magnetic fields due to Dirac particles in FRW spacetime

S. K. Sharma, P. R. Dhungel, U. Khanal

Some solutions of the Maxwell equations with Dirac particles for the source in FRW spacetime are discussed. The Green's function of the equation for the radial component of the Max…

astro-ph.CO2011

Effect of Massive Neutrino on Large Scale Structures

P. R. Dhungel, S. K. Sharma, U. Khanal

Jeans mass calculated with different combination of parameters involved has shown interesting variation with remarkable shifting of position of peak value from x = m/T = 0.5 to 5.5…

astro-ph.CO2011★ 8 cited

Perturbation of FRW Spacetime in NP Formalism

S. K. Sharma, U. Khanal

Perturbation of FRW spacetime is carried out in NP formalism. The equation governing the scalar, vector and tensor modes take on a very simple and transparent form. All of them can…

◍wovepaper

Papers, researchers and institutions, woven together.

Explore
  • Search
  • Researchers
  • Institutions
Account
  • Library
  • Chat
Data
  • arXiv.org
  • Semantic Scholar
  • OpenAlex
  • Latest RSS
AboutContactPrivacyDevelopersllms.txtopenapi.json
Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.