Phenomenological relation of coil to globule transition of polymer chain

Consider a polymer chain dissolved in a solvent, where its behavior is influenced by the Flory parameter, denoted by $\chi$. As the interaction parameter $\chi$ varies, the chain undergoes several conformational transitions:

• For $\chi > \chi_c$, the polymer collapses into a dense, globular structure with a radius of gyration scaling as $R_g \sim N^{1/3}$.

• At the critical point—commonly known as the $\theta$ point—where $\chi \sim \chi_c$, the chain behaves like an ideal random coil, characterized by $R_g \sim N^{1/2}$.

• In a good solvent, when $\chi < \chi_c$, the polymer chain is swollen and stretched, with $R_g \sim N^{3/5}$.

A “universal” expression that captures how the radius of gyration $R_g$ changes with $\chi$ is given by

  $R_g(\chi) = R_g^\mathrm{glob} + \frac{R_g^\mathrm{coil}-R_g^\mathrm{glob}}{1 + \exp[(\chi-\chi_c)/\Delta \chi]}$,

where $\Delta \chi$ quantifies the width of the conformational transition region and $\chi_c$ locates the transition.

To estimate the window width $\Delta \chi$, we first define an order parameter that measures deviations of the polymer’s size from its value at the $\theta$ point. We write

  $R = R_0 (1 + m)$,

with $R_0 \sim N^{1/2}b$, where $b$ is the monomer size and $m$ represents the fractional deviation from the ideal size.

Next, we expand the free energy $F(m)$ in powers of $m$. Close to the $\theta$ point, the expansion takes the form

  $\frac{F(m)}{k_BT} \simeq C_1 N (\chi-\chi_c) m^2 + C_2 N m^4 + \cdots$,

where $C_1$ and $C_2$ are constants, and $k_BT$ is the thermal energy.

In the mean-field (infinite-system) limit, the phase transition is sharp. However, for finite systems, fluctuations smear the transition, leading to a rounded behavior characterized by a finite width $\Delta \chi$ defined by $|\chi-\chi_c|$.

At the edge of the transition, the quadratic and quartic terms in the free energy become comparable. Equating these contributions gives

  $C_1 N\,\Delta\chi\,m^2 \sim C_2 N\,m^4,$

which implies

  $m^2 \sim \frac{C_1}{C_2}\,\Delta\chi$.

Furthermore, the transition is significantly broadened when the free energy barrier, estimated by the quartic term, is of the order of unity (in units of $k_BT$). That is, when

  $N C_2\, m^4 \sim O(1).$

Substituting our earlier estimate for $m^2$ into this condition, we obtain

  $N C_2 \left(\frac{C_1}{C_2}\Delta\chi\right)^2 \sim O(1),$

which simplifies to

  $\Delta\chi^2 \sim \frac{1}{N}.$

Thus, the rounding of the transition in terms of $\chi$ scales as

  $\Delta\chi \sim \frac{1}{\sqrt{N}}.$

HDR Moon 03-19-2025

Technical Approach:

Preparation of Source Images

  • Capture Three Photos:
    • Full Moon: Take a clear photograph of the full moon.
    • Two Waning Moons: Photograph the waning moon twice.
      • Overexposed Waning Moon: For one of the waning moon images, apply an exposure compensation of +3 levels to create an overexposed effect, which will enhance the halo effect around the moon.
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