Model Edwards AB

Arguments:

  • nu0 (float) - Excluded volume between all species \(\nu_0\)

  • delta_nuAB (float) - Extra excluded volume between A and B species \(\Delta \nu_{AB}\)

  • rho0 (float) - System density \(\rho_0\)

Example (python)

TODO

Example (json)

"model": {
  "type": "EdwardsAB",
  "Nref": 1.0,
  "bref": 1.0,
  "nu0": 40,
  "delta_nuAB": 10,
  "rho0": 3,
  "initfields": {
    "mu_minus": {
      "center0": [ 0 ],
      "height": 1.0,
      "ngaussian": 1,
      "type": "gaussians",
      "width": 0.1
    },
    "mu_plus": {
      "seed": 0,
      "type": "random"
    }
  }
},

Model Edwards AB Formalism

References: Park2020, Delaney2016

This is an extension of the Edwards model to include two species (A and B). This is very similar to the non-specific compressible model derived by Delaney2016 and the model derived by Park2020 in the absence of charges.

The model

\[\beta U(\pmb{r}) = \beta U_{bond}(\pmb{r}) + \beta U_{excl}\]

where

\[\beta U_{excl} = \frac{\nu_0}{2} \int d\pmb{r} (\bar{\rho}_A(\pmb{r}) + \bar{\rho}_B(\pmb{r}))^2 + \Delta \nu_{AB} \int d\pmb{r} \bar{\rho}_A(\pmb{r}) \bar{\rho}_B(\pmb{r}) + self interaction\]

where \(\bar{\rho}_K\) is the smeared density of species \(K\in{A,B}\) defined as \(\bar{\rho}_K = \Gamma_K * \hat{\rho}_K(\pmb{r}) = \int d\pmb{r} \Gamma_K (\pmb{r} - \pmb{r}') \hat{\rho}_K(\pmb{r}')\), where \(\Gamma_K(\pmb{r}) = \frac{1}{(2\pi a_K^2)^{3/2}} \exp{\left(-\frac{\lvert\pmb{r}\rvert}{2 a_K^2} \right)}\) is the smearing function and \(\hat{\rho}_K\) is the microscopic density.

To derive a field theory, we introduce the \(\bar{\rho}_+ = \bar{\rho}_A + \bar{\rho}_B\) and \(\bar{\rho}_- = \bar{\rho}_A - \bar{\rho}_B\). Following two Hubbard-Stratonovich transforms, the field theory derived for this model is

\[\mathcal{Z} = Z_0 \int \mathcal{D} w_+ \int \mathcal{D} w_- \exp{\left(-H[w_+,w_-]\right)}\]

where

\[H[w_+, w_-] = \frac{1}{2 \nu_0 + \Delta \nu_{AB}} \int d \pmb{r} [w_+(\pmb{r})]^2 + \frac{1}{\Delta \nu_{AB}} \int d \pmb{r} [w_-(\pmb{r})]^2 - \sum_p^P n_p \ln Q_p[\Gamma_A * w_A, \Gamma_B * w_B]\]

with \(w_A = i w_+ - w_-\) and \(w_B = i w_+ + w_-\). By introducing the following variables \(B_0=\frac{\nu_0 N^2}{R_{g0}^3}\), \(B_{AB}=\frac{\Delta \nu_{AB} N^2}{R_{g0}^3}\), \(C=\frac{\rho_0 R_{g0}}{N}\), \(\tilde{V} = \frac{V}{R_{g0}^3}\), \(\pmb{x} = \frac{\pmb{r}}{R_{g0}}\), \(n_p = \frac{C \tilde{V} \phi_p}{\alpha_p}\), \(\mu_+ = i w_+(\pmb{r}) N\), \(\mu_- = w_-(\pmb{r}) N\) (take a look at Duchs2014 if theres variables that were not defined), the field theory becomes

TODO: lots of these rescaling conventions are recycled from model to model. Can I combine into one place?

\[H[\mu_+, \mu_-] = - \frac{1}{2 B_0 + B_{AB}} \int d \pmb{x} [\mu_+(\pmb{x})]^2 + \frac{1}{B_{AB}} \int d \pmb{x} [\mu_-(\pmb{x})]^2 - C \tilde{V} \sum_p^P \frac{\phi_p}{\alpha_p} \ln Q_p[\Gamma_A * \mu_A, \Gamma_B * \mu_B]\]

The density operator of species K \(\varphi_K\) is (for a continuous chain)

\[\varphi_K (\pmb{x} ; [\mu]) = \sum_{p=1}^P \frac {\phi_p}{Q_p \alpha_p} \Gamma_K * \left( \int_{s \in K} ds q_p(x,s) q^\dagger_p(x,s) \right)\]

The forces are

\[\begin{split}\frac{\delta H[\mu_+,\mu_-]}{\delta \mu_+(\pmb{x})} &= - \frac{2}{2B_0 + B_{AB}} \mu_+(\pmb{x}) + C \left(\varphi_A(\pmb{x}) + \varphi_B(\pmb{x})\right)\\ \frac{\delta H[\mu_+,\mu_-]}{\delta \mu_-(\pmb{x})} &= \frac{2}{B_{AB}} \mu_-(\pmb{x}) + C \left(\varphi_B(\pmb{x}) - \varphi_A(\pmb{x})\right)\end{split}\]