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researcher

K. Knudsen

8 papers hereh-index 212 citations10 works total

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

author position
  • middle author7

Across the 7 of 8 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA7
  • astro-ph.SR1
same name
  • K. Knudsen — 73 papers, h 34
  • K. Knudsen — 31 papers, h 10
  • K. Knudsen — 22 papers, h 10
  • K. Knudsen — 20 papers, h 17
  • K. Knudsen — 2 papers, h 29
  • K. Knudsen — 1 paper, h 1

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
20242026
most citedAccurate sticking coefficient calculation for carbonaceous dust growth through accretion and desorption in astrophysical environments

12 citations · 13 across the 8 of their papers we have counts for

collaborators
Showing 2026Show all

3 papers · 1 filter

astro-ph.GA2026

From stardust to interstellar grain growth in the first galaxies: a cosmological transition in dust evolution near z ~ 8.9

Denis Burgarella, Tom J. L. C. Bakx, Raffaella Schneider +7

When and how did dust begin to shape galaxies? Motivated by the identification of an apparent redshift break in galaxy dust masses, suggesting substantially lower dust masses at $z…

astro-ph.GA2026

Efficient Interstellar Grain Growth from High Sticking Coefficients on Amorphous Carbon Dust

Clarke J. Esmerian, Duncan Bossion, Francois Dulieu +8

Cosmic dust is the solid phase of the interstellar medium (ISM), classically assumed to be composed of carbonaceous and silicate grains with size distributions spanning ∼5 A˚…

astro-ph.GA2026

Silicate cosmic dust grain collisions in the interstellar medium: A molecular dynamics study

C. J. Esmerian, S. R. Hashemi, W. M. C. Sameera +7

(abridged) We aim to predict the most important parameters for grain-grain collision outcomes in models of interstellar grain population evolution: the threshold velocities for sha…

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