computational-physics-guide
Computational physics methods, simulations, and research tools
Best use case
computational-physics-guide is best used when you need a repeatable AI agent workflow instead of a one-off prompt.
Computational physics methods, simulations, and research tools
Teams using computational-physics-guide should expect a more consistent output, faster repeated execution, less prompt rewriting.
When to use this skill
- You want a reusable workflow that can be run more than once with consistent structure.
When not to use this skill
- You only need a quick one-off answer and do not need a reusable workflow.
- You cannot install or maintain the underlying files, dependencies, or repository context.
Installation
Claude Code / Cursor / Codex
Manual Installation
- Download SKILL.md from GitHub
- Place it in
.claude/skills/computational-physics-guide/SKILL.mdinside your project - Restart your AI agent — it will auto-discover the skill
How computational-physics-guide Compares
| Feature / Agent | computational-physics-guide | Standard Approach |
|---|---|---|
| Platform Support | Not specified | Limited / Varies |
| Context Awareness | High | Baseline |
| Installation Complexity | Unknown | N/A |
Frequently Asked Questions
What does this skill do?
Computational physics methods, simulations, and research tools
Where can I find the source code?
You can find the source code on GitHub using the link provided at the top of the page.
SKILL.md Source
# Computational Physics Guide
Apply computational methods to physics research, including molecular dynamics, Monte Carlo simulations, quantum computing, and numerical methods for solving physical systems.
## Computational Methods Overview
| Method | Application | Scale | Key Software |
|--------|-------------|-------|-------------|
| **Molecular Dynamics (MD)** | Atomic-scale dynamics, materials | Atoms-molecules | LAMMPS, GROMACS, NAMD |
| **Density Functional Theory (DFT)** | Electronic structure, quantum chemistry | Electrons | VASP, Gaussian, Quantum ESPRESSO |
| **Monte Carlo (MC)** | Statistical mechanics, phase transitions | Configurable | Custom, CASINO |
| **Finite Element Method (FEM)** | Continuum mechanics, electrostatics | Macroscopic | COMSOL, FEniCS, Abaqus |
| **Finite Difference (FDTD)** | Electrodynamics, wave propagation | Macroscopic | Meep, Lumerical |
| **N-body Simulation** | Gravitational dynamics, plasma | Stars/particles | GADGET, REBOUND |
| **Lattice QCD** | Quantum chromodynamics | Subatomic | MILC, openQCD |
## Molecular Dynamics
### Basic MD Algorithm
```python
import numpy as np
def lennard_jones(r, epsilon=1.0, sigma=1.0):
"""Lennard-Jones potential and force."""
r6 = (sigma / r) ** 6
r12 = r6 ** 2
potential = 4 * epsilon * (r12 - r6)
force = 24 * epsilon * (2 * r12 - r6) / r
return potential, force
def velocity_verlet(positions, velocities, forces, masses, dt):
"""Velocity Verlet integration step."""
# Half-step velocity update
velocities += 0.5 * forces / masses * dt
# Full-step position update
positions += velocities * dt
# Compute new forces
new_forces = compute_forces(positions)
# Complete velocity update
velocities += 0.5 * new_forces / masses * dt
return positions, velocities, new_forces
def md_simulation(n_atoms, n_steps, dt=0.001, temperature=1.0):
"""Simple NVE molecular dynamics simulation."""
# Initialize positions on a grid
positions = initialize_fcc_lattice(n_atoms, box_size=10.0)
velocities = np.random.randn(n_atoms, 3) * np.sqrt(temperature)
velocities -= velocities.mean(axis=0) # Remove center of mass motion
forces = compute_forces(positions)
trajectory = []
for step in range(n_steps):
positions, velocities, forces = velocity_verlet(
positions, velocities, forces,
masses=np.ones(n_atoms), dt=dt
)
if step % 100 == 0:
ke = 0.5 * np.sum(velocities**2)
pe = compute_potential_energy(positions)
print(f"Step {step}: KE={ke:.4f}, PE={pe:.4f}, Total={ke+pe:.4f}")
trajectory.append(positions.copy())
return trajectory
```
### LAMMPS Input Script Example
```
# LAMMPS input: Lennard-Jones fluid simulation
units lj
atom_style atomic
boundary p p p
# Create simulation box and atoms
lattice fcc 0.8442
region box block 0 10 0 10 0 10
create_box 1 box
create_atoms 1 box
# Set mass and interactions
mass 1 1.0
pair_style lj/cut 2.5
pair_coeff 1 1 1.0 1.0 2.5
# Initialize velocities at T=1.0
velocity all create 1.0 87287 dist gaussian
# Thermostat: Nose-Hoover NVT
fix 1 all nvt temp 1.0 1.0 0.1
# Output settings
thermo 100
thermo_style custom step temp pe ke etotal press
dump 1 all custom 1000 trajectory.lammpstrj id x y z vx vy vz
# Run simulation
timestep 0.005
run 100000
```
## Monte Carlo Methods
### Metropolis Algorithm for Ising Model
```python
import numpy as np
def ising_monte_carlo(L, temperature, n_steps):
"""2D Ising model simulation using Metropolis algorithm."""
# Initialize random spin configuration
spins = np.random.choice([-1, 1], size=(L, L))
beta = 1.0 / temperature
energies = []
magnetizations = []
for step in range(n_steps):
for _ in range(L * L): # One sweep = L^2 single spin flips
# Choose random spin
i, j = np.random.randint(0, L, size=2)
# Calculate energy change for flipping spin (i,j)
neighbors = (
spins[(i+1)%L, j] + spins[(i-1)%L, j] +
spins[i, (j+1)%L] + spins[i, (j-1)%L]
)
delta_E = 2 * spins[i, j] * neighbors
# Metropolis acceptance criterion
if delta_E <= 0 or np.random.random() < np.exp(-beta * delta_E):
spins[i, j] *= -1
# Measure observables
if step % 10 == 0:
E = -np.sum(spins * (np.roll(spins, 1, 0) + np.roll(spins, 1, 1)))
M = np.abs(np.sum(spins))
energies.append(E / L**2)
magnetizations.append(M / L**2)
return energies, magnetizations
# Run near the critical temperature (T_c ≈ 2.269 for 2D Ising)
E, M = ising_monte_carlo(L=32, temperature=2.269, n_steps=10000)
print(f"Mean energy: {np.mean(E[-100:]):.4f}")
print(f"Mean magnetization: {np.mean(M[-100:]):.4f}")
```
## Density Functional Theory
### Quantum ESPRESSO Workflow
```bash
# Step 1: Self-consistent field (SCF) calculation
cat > si_scf.in << 'EOF'
&CONTROL
calculation = 'scf'
prefix = 'silicon'
outdir = './tmp/'
pseudo_dir = './pseudo/'
/
&SYSTEM
ibrav = 2
celldm(1) = 10.26 ! Lattice constant in Bohr
nat = 2
ntyp = 1
ecutwfc = 30.0 ! Kinetic energy cutoff (Ry)
ecutrho = 300.0 ! Charge density cutoff (Ry)
/
&ELECTRONS
conv_thr = 1.0d-8
/
ATOMIC_SPECIES
Si 28.086 Si.pbe-n-rrkjus_psl.1.0.0.UPF
ATOMIC_POSITIONS crystal
Si 0.00 0.00 0.00
Si 0.25 0.25 0.25
K_POINTS automatic
8 8 8 0 0 0
EOF
pw.x < si_scf.in > si_scf.out
# Step 2: Band structure calculation
# (requires nscf + bands post-processing)
```
### Python Interface (ASE + GPAW)
```python
from ase.build import bulk
from gpaw import GPAW, PW
# Create silicon crystal structure
si = bulk('Si', 'diamond', a=5.43)
# DFT calculation with GPAW
calc = GPAW(mode=PW(300), # Plane-wave cutoff: 300 eV
kpts=(8, 8, 8), # k-point mesh
xc='PBE', # Exchange-correlation functional
txt='si_gpaw.txt') # Output file
si.calc = calc
energy = si.get_potential_energy()
print(f"Total energy: {energy:.4f} eV")
print(f"Energy per atom: {energy/len(si):.4f} eV")
# Equation of state (find equilibrium lattice constant)
from ase.eos import EquationOfState
volumes, energies = [], []
for a in np.linspace(5.3, 5.6, 10):
si = bulk('Si', 'diamond', a=a)
si.calc = GPAW(mode=PW(300), kpts=(8,8,8), xc='PBE', txt=None)
volumes.append(si.get_volume())
energies.append(si.get_potential_energy())
eos = EquationOfState(volumes, energies)
v0, e0, B = eos.fit()
print(f"Equilibrium volume: {v0:.2f} A^3, Bulk modulus: {B:.1f} GPa")
```
## Numerical Methods
### Solving ODEs (Runge-Kutta)
```python
from scipy.integrate import solve_ivp
import matplotlib.pyplot as plt
# Example: Damped harmonic oscillator
# m*x'' + gamma*x' + k*x = 0
def damped_oscillator(t, y, gamma=0.1, omega0=1.0):
x, v = y
dxdt = v
dvdt = -2*gamma*v - omega0**2 * x
return [dxdt, dvdt]
sol = solve_ivp(damped_oscillator, [0, 50], [1.0, 0.0],
t_eval=np.linspace(0, 50, 1000),
method='RK45', rtol=1e-10)
plt.plot(sol.t, sol.y[0])
plt.xlabel('Time')
plt.ylabel('Displacement')
plt.title('Damped Harmonic Oscillator')
plt.savefig('oscillator.pdf', dpi=300)
```
### Solving PDEs (Finite Differences)
```python
# 2D Heat equation: du/dt = alpha * (d2u/dx2 + d2u/dy2)
def heat_equation_2d(Nx, Ny, Nt, alpha=0.01, dt=0.001):
dx = dy = 1.0 / max(Nx, Ny)
u = np.zeros((Nx, Ny))
u[Nx//4:3*Nx//4, Ny//4:3*Ny//4] = 1.0 # Initial hot region
for t in range(Nt):
u_new = u.copy()
u_new[1:-1, 1:-1] = u[1:-1, 1:-1] + alpha * dt / dx**2 * (
u[2:, 1:-1] + u[:-2, 1:-1] + u[1:-1, 2:] + u[1:-1, :-2]
- 4 * u[1:-1, 1:-1]
)
u = u_new
return u
```
## HPC and Parallelization
| Approach | Tool | Best For |
|----------|------|----------|
| Shared memory (threads) | OpenMP | Multi-core CPU parallelism |
| Distributed memory (MPI) | mpi4py, MPI | Multi-node cluster computing |
| GPU computing | CUDA, CuPy, JAX | Massively parallel computations |
| Workflow management | Snakemake, Nextflow | Complex simulation pipelines |
| Job scheduling | SLURM, PBS | HPC cluster job submission |
## Research Resources
| Resource | Description |
|----------|-------------|
| arXiv cond-mat | Condensed matter preprints |
| arXiv hep-lat | Lattice field theory preprints |
| Journal of Computational Physics | Top computational physics journal |
| Physical Review E | Statistical, nonlinear, soft matter |
| Computer Physics Communications | Methods + software papers |
| NIST databases | Physical constants, atomic data |Related Skills
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