Based on:
With:
Mark Hindmarsh
Anna Kormu
Asier Lopez-Eiguren
Kari Rummukainen
Motivation
Necklaces are networks of strings carrying monopoles.
Models can be embedded in
GUTs, including $\mathrm{SO}(10)$.
Might behave differently
to strings - role of monopoles?
Observations:
Cosmic ray and $\gamma$-ray
signals? astro-ph/9704257
Gravitational waves? (or lack thereof)
The model
"$\mathrm{SU}(2)$ Georgi-Glashow model with two
adjoint Higgses"
$$ \begin{multline} V(\Phi_1,\Phi_2) = - m_1^2\mathrm{Tr}\Phi_1^2 -
m_2^2\mathrm{Tr}\Phi_2^2 \\ +\lambda
(\mathrm{Tr}\Phi_1^2)^2 + \lambda
(\mathrm{Tr}\Phi_2^2)^2
+\kappa(\mathrm{Tr}\Phi_1\Phi_2)^2. \end{multline} $$
with $\Phi_n^a = \phi_n^a\sigma^a/2$ and the usual
action.
If $m_1^2 > m_2^2$, get necklaces with monopoles, charge $\{\pm 1\}$.
If $m_1^2 =
m_2^2$, behaviour depends on $\kappa/2\lambda$:
If $\kappa = 2\lambda$, there's a global
$\mathrm{U}(1)$ - superfluidity.
If $\kappa \neq 2\lambda$, monopoles split into two
semipoles with complex charge $\{1,i,-1,-i\}$.
Necklaces
When $m_1^2 > m_2^2$, $\mathrm{U}(1)$ breaks to $Z_2$
Strings form, joining up the monopoles
Semipoles 1
When $m_1^2 = m_2^2$ and $\kappa/2\lambda < 1$, get
semipoles.
Four types of pole, with complex charge $\{1, i, -1,
-i\}$.
Linked by four types of string, with complexified flux
$\Phi_B^{(1)} + i \Phi_B^{(2)} \in \{1 + i, -1 + i, -1 - i,
1 - i\}$.
Semipoles 2
When $m_1^2 = m_2^2$ and $\kappa/2\lambda > 1$, slight
difference...
Vacua rotated by 45° so string fields are rotated,
too,
$$\Phi_\pm = (\Phi_1 \pm \Phi_2)/\sqrt{2}.$$
Special case
When $m_1^2 = m_2^2$ and $\kappa/2\lambda = 1$, there
is a global $\mathrm{U}(1)$.
(We won't look at this any further today...)
Implementing the simulations
Real-time lattice simulation,
temporal gauge ($A^0 = 0$).
Initial conditions and evolution must satisfy Gauss law.
Fundamental quantities: links $U_i \in
\mathrm{SU}(2)$ and fields $\Phi_n$.
Our key measurements are the location of monopoles and
plaquettes with winding number.
Getting the monopoles
Make projectors $\Pi_\pm =
\frac{1}{2} (1 \pm \hat{\Phi}_1)$ where $$\hat{\Phi}_1 = \Phi_1\sqrt{2/\mathrm{Tr}\, \Phi_1^2}$$
Get the $\mathrm{U}(1)$ gauge field corresponding to $\Phi_1$,
$$ u_\mu(x) = \Pi_+(x) U_\mu(x) \Pi_+(x+\hat{\mu}). $$
Construct an effective "field strength tensor" hep-lat/0009037
$$ \alpha_{\mu\nu}
= \frac{2}{g} \; \mathrm{arg} \; \mathrm{Tr}\; u_\mu(x) u_\nu(x+\hat{\mu}) u_\mu^\dagger(x+\hat{\nu}) u_\nu^\dagger(x). $$
From which effective magnetic field and charge is
$$B_i = \frac{1}{2} \epsilon_{ijk} \alpha_{jk}; \qquad \rho_{\mathrm{M}}= \sum_{i=1}^3 [B_i(x+\hat{\imath}) - B_i(x)] $$
Getting the winding
Similar to Abelian
Higgs hep-ph/9809334
Difference in phase angle for $\Phi_2$ hep-lat/0009037
$$\begin{multline}\delta_i(x) = \mathrm{arg} \; \mathrm{Tr} \; \big[ \hat{\Phi_2}(x) \Pi_-(x) U_i(x) \Pi_-(x+\hat{\imath}) \\
\hat{\Phi_2}(x +\hat{\imath}) \Pi_+(x+\hat{\imath}) U_i^\dagger(x) \Pi_+(x)
\big]. \end{multline}$$
Winding number through a plaquette in the $ij$-plane at
$x$ is then
$$Y_{ij}(x) = \delta_i(x) + \delta_j(x+\hat{\imath})
- \delta_i(x+\hat{\jmath}) - \delta_j(x) - g \alpha_{ij}(x). $$
We can trace this (and the monopoles) through the
lattice.
Or in other words
✅ Yes, we can obtain the residual $\mathrm{U}(1)$ field.
✅ Yes, we can measure the vortex winding associated with
the other Higgs field.
✅ Yes, they're both gauge invariant.
For necklaces, the heavier field (wlog $\Phi_1$)
forms monopoles.
For semipoles, we have to make two magnetic fields,
either $\mathbf{B}^{(1)}$ and $\mathbf{B}^{(2)}$ from
$\Phi_1$ and $\Phi_2$
or $\mathbf{B}^{(\pm)}$ from
$\Phi^{(\pm)} = \frac{1}{\sqrt{2}}(\Phi_1 \pm \Phi_2)$.
String and pole position movie
Video credit: Asier Lopez-Eiguren
Running the simulations
"Naive" random initial conditions (memory soon lost).
Simulate physical equations of motion, but first:
Some smoothing
$$ \Phi_n(\mathbf{x}) \to \frac{1}{12} \sum_i \left[
\Phi_n(\mathbf{x}-\hat{\imath}) + 2\Phi_n(\mathbf{x}) +
\Phi_n(\mathbf{x} + \hat{\imath}) \right]. $$
Then some heavy damping in a Minkowski
background.
And 'core growth' (run equations with
$s=-1$).
$1920^3$ lattices, run for one light crossing
time.
Gauss Law OK, energy conservation < 1%.
Limitations of the simulations
(in addition to the usual caveats for field theory strings)
Mass scales $m_1^2$ and $m_2^2$ will never be that
different 😕
Largest we have is $m_2^2/m_1^2 = 0.04$.
Decrease $m_2$? Fatter strings reduce
statistics.
Decrease $m_2$? Defect formation dynamics happens
on time $1/m_2$ - need longer simulations. Light
crossing time?
Increase $m_1$? Smaller monopoles risk pinning on
lattice.
Movie interlude
(We also have 3D
and 360 movies!)
Semipoles 1 ($\kappa/2\lambda < 1$)
Semipoles 2 ($\kappa/2\lambda > 1$)
(note, isosurfaces of unrotated $\Phi_1$, $\Phi_2$)
Dynamics: key quantities
Lattice projectors give the positions of monopoles
(total $N$) and plaquettes with winding (total $L$).
Average defect separations in volume $V$
$$\xi_\mathrm{m} = \left(\frac{V}{N}\right)^{1/3};
\qquad \xi_\mathrm{s} = \left(\frac{V}{L}\right)^{1/2}.$$
Comoving pole density
$$ n = \frac{\xi_\mathrm{s}^2}{\xi_\mathrm{m}^3}. $$
Energy, Lagrangian-derived measures less
successful 🤷♂️.
$\xi_\mathrm{s}$ and $\xi_\mathrm{m}$ - necklaces
String separation: linear scaling with conformal
time $\tau$.
Monopole separation: $\xi_m \mathrm
\propto{\tau}^{2/3}$.
No real dependence on initial $\xi_\mathrm{m}$.
$\xi_\mathrm{s}$ and $\xi_\mathrm{m}$ - semipoles
Same general story as for necklaces.
Some hints of different $\kappa/2\lambda$
behaviour...
Monopole linear density - necklaces and semipoles
Note 'pseudopoles': projecting wrong
complexified $\mathbf{B}$ fields.
Everything physical goes to constant $n$ (more or
less).
Conclusion
Large simulations of necklaces in radiation
era: 10M CPUh.
Both standard and semipole necklaces.
String separation scales with
conformal time: $\xi_\mathrm{s} \propto \tau$.
But comoving pole separation $n$ along strings is
constant
⇒ Monopoles are "along for the ride"...
Models in the literature don't quite work.
More information