Driving Forces for Cell Cluster Shape Evolution and Stability Asha - - PowerPoint PPT Presentation

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Driving Forces for Cell Cluster Shape Evolution and Stability Asha - - PowerPoint PPT Presentation

Driving Forces for Cell Cluster Shape Evolution and Stability Asha Nurse, L.B. Freund and J. Youssef School of Engineering, Brown University Applied and Computational Mathematics Seminar Series 04/19/2011 Acknowledgment. This work is supported


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Driving Forces for Cell Cluster Shape Evolution and Stability

  • Acknowledgment. This work is supported primarily by the MRSEC Program of the National

Science Foundation at Brown University under award DMR-0520651.

Asha Nurse, L.B. Freund and J. Youssef School of Engineering, Brown University Applied and Computational Mathematics Seminar Series 04/19/2011

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  • The Model

– Experimental Background

– Origin of Surface Energy – Analysis of the Model – Results & Conclusions

  • Linear Stability of a Toroidal Cluster

– Stability Analysis – Formulation of Model

  • Calculating Surface Area and Volume of Perturbed shape
  • Alternate Perturbed Shape

– Non-constant Surface Energy Density – Results & Conclusions

Outline

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Dean, D. M., Napolitano, A. P., Youssef, J. and Morgan, J. R. FASEB 2007

Directed Self Assembly Experiments

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The Phenomenon

800 μm cell suspension polyacrylimide chamber solvent toroidal cluster

A mathematical model of the current system will

  • 1. allow for understanding the factors involved in cell

cluster reorganization

  • 2. offer a framework to organize lab observations
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SLIDE 5

Spontaneous Climb

200μm

2 hrs 4 hrs 6 hrs

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The Model

Nurse, A., Youssef, J., Freund, L.B. JAM 2011 Under Review

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Possible Origin of Surface Energy

Higher free energy tension bundles

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The Model

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Finding the Surface Flux

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A Variational Approach

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κ = 15 20 25

β(τ) a(τ)/b0 β(τ) α(τ)/b0 κ = 25 ω =100

τ Numerical Solution for Shape Evolution

κ = κeq

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β(τ) α(τ)/b0 κ = 25 ω =100

τ

κ = 15 20 25

β(τ) a(τ)/b0

Numerical Solution for Shape Evolution

κ = κeq

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α = 85 65 55

a(τ)/b0 β(τ)

τ Numerical Solution for shape evolution

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Extraction of Surface Energy Density Values

time (hrs) γ (mJ/m2) ms 10-14 (m4hr/g) 2 0.0580 0.543 4 0.0638 0.920 6 0.0667 1.238 8 0.0693 1.386 α1= 55°, α2 = 65°

Foty & Steinberg (05) & Sivansankar et al (99): 1.556 x 10-4 ≤ γ ≤ 1.522 x 10-3 mJ/m2

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Conclusions from the Basic Model

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Outline

  • The Model

– Experimental Background – Origin of Surface Energy – Riemannian Geometry – Analysis of the Model – Results & Conclusions

  • Linear Stability of a Toroidal Cluster

– Stability Analysis – Formulation of Model

  • Calculating Surface Area of Perturbed shape
  • Alternate Perturbed Shape

– Non-constant Surface Energy Density – Results & Conclusions

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Stability of Toroidal Shapes

McGraw et al, Soft Matter 2010 Pairam & Fernandez-Nieves, Physics Rev. Letter 2009 a0/ b0 ≈ 1.9 a0/ b0 ≈ 8.7 Jeff Morgan Lab

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Linear Stability Analysis of the Toroidal Cluster

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Linear Stability Analysis of the Toroidal Cluster

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γ is spatially constant

Always stable

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Alternate perturbed shape

Inconclusive

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a0 r0

γ is not spatially constant

a0 r0

θ

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r0/b0 = 4

stable unstable

Nonuniform γ with same applied perturbation

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r0/b0 = 4

stable unstable

Non uniform γ with same applied perturbation

r0/b0 = 8

stable unstable

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γ is a function of position on the surface

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Conclusions on Toroidal Stability

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Summary of Results on Toroidal Clusters

Formation of uniform toroidal self-assembled cluster at base of chamber Cluster spontaneously climbs conical pillar to reduce its surface area Remains at base of chamber undergoes localized thinning around circumference For family of applied perturbation

  • γ must be a variable
  • γ (θ) sufficient for instability
  • r0/b0 affects cluster stability

Rate of climb affected by

  • influence of SE/GPE (κ)
  • slope of conical pillar (α)
  • surface mobility of diffusing cells
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  • Origin of γ requires further investigation
  • More precise method required to extract values of ms
  • Conduct linear stability analysis of toroidal shapes with

– other family of perturbations – more complex surface energy density function

  • For spatially constant γ, conduct a nonlinear stability analysis of the

toroidal clusters

Further Work and Questions

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Acknowledgements & Publications

200 μm

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