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Updated: Jun 8, 2026

SNARE-mediated Fusion of Single Proteoliposomes with Tethered Supported Bilayers in a Microfluidic Flow Cell Monitored by Polarized TIRF Microscopy
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Merging and fragmentation in the Burgers dynamics.

Francis Bernardeau1, Patrick Valageas

  • 1Institut de Physique Théorique, CEA/DSM/IPhT, Unité de recherche associée au CNRS, CEA/Saclay, Gif-sur-Yvette, France.

Physical Review. E, Statistical, Nonlinear, and Soft Matter Physics
|September 28, 2010
PubMed
Summary
This summary is machine-generated.

We investigate the adhesion model in cosmology, revealing that halo fragmentation occurs in 2D and higher dimensions. Pointlike halos merge via three-body collisions, leading to continuous halo formation through fragmentation and merging.

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Area of Science:

  • Cosmology
  • Astrophysics
  • Fluid Dynamics

Background:

  • The adhesion model describes large-scale structure formation in the universe.
  • Previous studies focused on specific aspects of this model.

Purpose of the Study:

  • To explore noiseless Burgers dynamics in the inviscid limit using a geometrical model.
  • To analyze matter distribution and space partitions within this framework.

Main Methods:

  • Utilizing a geometrical model based on Legendre transforms and convex hulls.
  • Analyzing matter evolution within the shock manifold.
  • Investigating Lagrangian space triangulation and Eulerian space tessellation.

Main Results:

  • Halo mass distribution arises from Lagrangian space triangulation.
  • Eulerian space tessellation defines empty regions with shock nodes.
  • Halo fragmentation occurs in dimensions >= 2.
  • Pointlike halos merge via three-body collisions; two-body collisions create new shock nodes.

Conclusions:

  • The geometrical model provides insights into halo fragmentation and merging dynamics.
  • This leads to a continuous formation of massive halos.
  • The findings generalize to higher spatial dimensions.