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classical-mechanics

Newtonian mechanics including Lagrangian and Hamiltonian dynamics, central forces, rigid body motion, small oscillations, and chaos theory for physics applications.

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Repository
NeuralBlitz/Agent-Gateway
Letzte Quellaktivität
9. April 2026 um 10:58
Erkannte Sprache von SKILL.md
Englisch
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1
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0

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SKILL.md
Quellanweisungen · Schreibgeschützte Vorschau
name
Classical Mechanics
description
Newtonian mechanics including Lagrangian and Hamiltonian dynamics, central forces, rigid body motion, small oscillations, and chaos theory for physics applications.
license
MIT
compatibility
python>=3.8
audience
physicists, engineers, researchers, students
category
physics
# Classical Mechanics ## What I Do I provide comprehensive classical mechanics tools including Newtonian dynamics, Lagrangian and Hamiltonian formulations, central force problems, rigid body dynamics, small oscillations, and celestial mechanics for physics applications. ## When to Use Me - Particle and rigid body dynamics - Orbital mechanics calculations - Vibrational analysis - Conservative system analysis - Collision and impact problems - Celestial mechanics ## Core Concepts - **Newton's Laws**: Force, mass, acceleration relationships - **Lagrangian Mechanics**: Generalized coordinates, Euler-Lagrange - **Hamiltonian Mechanics**: Phase space, canonical equations - **Central Forces**: Gravitational, inverse-square laws - **Rigid Body Dynamics**: Moments of inertia, Euler equations - **Small Oscillations**: Normal modes, normal coordinates - **Canonical Transformations**: Point, contact transformations - **Action Principles**: Hamilton's principle, variational methods ## Code Examples ### Newtonian Dynamics ```python import numpy as np def newton_force(m, a): return m * a def gravitational_force(m1, m2, r): G = 6.674e-11 return G * m1 * m2 / r**2 def orbital_velocity(m, r, M): return np.sqrt(G * M / r) G = 6.674e-11 m = 5.972e24 # Earth mass r = 6.371e6 # Earth radius v = orbital_velocity(m, r, m) print(f"Orbital velocity: {v:.2f} m/s") def projectile_motion(v0, theta, h0=0, g=9.81): vx = v0 * np.cos(theta) vy = v0 * np.sin(theta) t_flight = (vy + np.sqrt(vy**2 + 2*g*h0)) / g R = vx * t_flight H = h0 + vy**2 / (2*g) return R, H, t_flight ``` ### Lagrangian Mechanics ```python from sympy import symbols, Function, diff t = symbols('t') q = Function('q')(t) q_dot = diff(q, t) q_ddot = diff(q_dot, t) def lagrangian_example(m, k, q, q_dot): T = 0.5 * m * q_dot**2 V = 0.5 * k * q**2 return T - V def euler_lagrange(L, q, t): q_dot = diff(q, t) dL_dq = diff(L, q) dL_dqdot = diff(L, q_dot) ddt_dL_dqdot = diff(dL_dqdot, t) return ddt_dL_dqdot - dL_dq m, k = symbols('m k') L = lagrangian_example(m, k, q, q_dot) print(f"Lagrangian: {L}") ``` ### Central Force Motion ```python def effective_potential(r, L, m, U): return U + L**2 / (2 * m * r**2) def orbital_equation(r, theta, E, L, m, mu, k): u = 1 / r du_dtheta = -1 / r**2 * dr_dtheta return du_dtheta + u - mu * k / L**2 def eccentricity(E, L, m, k): return np.sqrt(1 + 2 * E * L**2 / (m * k**2)) m_earth = 5.972e24 L = 2.66e40 e = eccentricity(-5e7, L, m_earth, 3.98e14) print(f"Orbital eccentricity: {e:.4f}") ``` ### Rigid Body Dynamics ```python def moment_of_inertia(parallel_axis, m, d): return parallel_axis + m * d**2 def angular_momentum(I, omega): return I * omega def rotational_kinetic_energy(I, omega): return 0.5 * I * omega**2 I_cm = 0.5 * m * r**2 # Solid sphere I_axis = moment_of_inertia(I_cm, m, r) print(f"Parallel axis I: {I_axis:.4e} kg·m²") def euler_equations(I1, I2, I3, omega1, omega2, omega3): I1_dot = (I2 - I3) * omega2 * omega3 / I1 I2_dot = (I3 - I1) * omega3 * omega1 / I2 I3_dot = (I1 - I2) * omega1 * omega2 / I3 return I1_dot, I2_dot, I3_dot ``` ### Small Oscillations ```python def normal_modes(k_matrix, m_matrix): eigvals, eigvecs = np.linalg.eig(np.linalg.inv(m_matrix) @ k_matrix) return np.sqrt(eigvals), eigvecs def natural_frequencies(k, m): omega_1 = np.sqrt(k / m) omega_2 = np.sqrt(3 * k / m) return omega_1, omega_2 k_matrix = np.array([[2, -1], [-1, 1]]) m_matrix = np.eye(2) frequencies, modes = normal_modes(k_matrix, m_matrix) print(f"Normal frequencies: {frequencies}") print(f"Mode shapes:\n{modes}") ``` ## Best Practices 1. **Conserved Quantities**: Identify symmetries and conserved quantities 2. **Degrees of Freedom**: Choose appropriate generalized coordinates 3. **Small Oscillations**: Check linear approximation validity 4. **Integrals of Motion**: Use energy, momentum conservation 5. **Phase Space**: Consider Hamiltonian for complex systems ## Common Patterns ```python # Symplectic integrator def symplectic_integrator(H, q0, p0, dt, n_steps): q = np.zeros((n_steps + 1, len(q0))) p = np.zeros((n_steps + 1, len(p0))) q[0], p[0] = q0, p0 for i in range(n_steps): p[i+1] = p[i] - dt * H.diff('q').subs(zip(q[i], p[i])) q[i+1] = q[i] + dt * H.diff('p').subs(zip(q[i], p[i+1])) return q, p # Verlet algorithm for molecular dynamics def verlet_position(r, v, a, dt): return 2*r - r_prev + a*dt**2 ``` ## Core Competencies 1. Lagrangian and Hamiltonian mechanics 2. Central force and orbital problems 3. Rigid body dynamics 4. Small oscillations and normal modes 5. Variational principles
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