Carl H. Gibson (Univ. Cal. San Diego)

Identifiers

• name variant Carl H. Gibson (Univ. Cal. San Diego) 0.60 · backfill

Papers (9)

1. Why are so many primitive stars observed in the Galaxy halo? physics.gen-ph · 2012 · author #1
2. Formation of Planets by Hydrogravitational Dynamics astro-ph.CO · 2010 · author #1
3. Turbulence and turbulent mixing in natural fluids astro-ph.CO · 2010 · author #1
4. The Origin of Life from Primordial Planets astro-ph.CO · 2010 · author #1
5. Planets and Dark Energy astro-ph · 2008 · author #1
6. Hydro-Gravitational-Dynamics Interpretation of the Tadpole VV29 Merging Galaxy System: Dark-Matter-Halo-Planet Star-Cluster Wakes astro-ph · 2008 · author #1
7. Evidence for Hydro-Gravitational Structure Formation Theory versus Cold-Dark-Matter, Hierarchical-Clustering, and Jeans 1902 astro-ph · 2003 · author #1
8. Planck-Kerr Turbulence astro-ph · 2003 · author #1
9. Turbulence and diffusion: fossil turbulence astro-ph · 2000 · author #1

Mentions

• 1206.0187 #1 · backfill · confidence 0.70 Carl H. Gibson (Univ. Cal. San Diego)
• 1012.5522 #1 · backfill · confidence 0.70 Carl H. Gibson (Univ. Cal. San Diego)
• 1005.2772 #1 · backfill · confidence 0.70 Carl H. Gibson (Univ. Cal. San Diego)
• 1004.0504 #1 · backfill · confidence 0.70 Carl H. Gibson (Univ. Cal. San Diego)
• 0803.4293 #1 · backfill · confidence 0.70 Carl H. Gibson (Univ. Cal. San Diego)
• 0803.4288 #1 · backfill · confidence 0.70 Carl H. Gibson (Univ. Cal. San Diego)

Frequent Coauthors

• Rudolph E. Schild (Harvard) 2 shared papers
• Rudolph E. Schild (Harvard Univ.) 2 shared papers
• N. C. Wickramasinghe (Cardiff Univ.) 1 shared papers
• Rudy Schild (Harvard) 1 shared papers
• Theo M. Nieuwenhuizen (Amsterdam University) 1 shared papers