1
2
3
4
5
6
7
8
9
10
11
12
13
14
15
16
17
18
19
20
21
22
23
24
25
26
27
28
29
30
31
32
33
34
35
36
37
38
39
40
41
42
43
44
45
46
47
48
49
50
51
52
53
54
55
56
57
58
59
60
61
62
63
64
65
66
67
68
69
70
71
72
73
74
75
76
77
78
79
80
81
82
83
84
85
86
87
88
89
90
91
92
93
94
95
96
97
98
99
100
101
102
103
104
105
106
107
108
109
110
111
112
113
114
115
116
117
118
119
120
121
122
123
124
125
126
127
128
129
130
131
132
133
134
135
136
137
138
139
140
141
142
143
144
145
146
147
148
149
150
151
152
153
154
155
156
157
158
159
160
161
162
163
164
165
166
167
168
169
170
171
172
173
174
175
176
177
178
179
180
181
182
183
184
185
186
187
188
189
190
191
192
193
194
195
196
197
198
199
200
201
202
203
204
205
206
207
208
209
210
211
212
213
214
215
216
217
218
219
220
221
222
223
224
225
226
227
228
229
230
231
232
233
234
235
236
237
238
239
240
241
242
243
244
245
246
247
248
249
250
251
252
253
254
255
256
257
258
259
260
261
262
263
264
265
266
267
268
269
270
271
272
273
274
275
276
277
278
279
280
281
282
283
//! Lagrangian Dynamics — derive equations of motion for mechanical systems.
//!
//! Demonstrates:
//! - Simple pendulum: Euler–Lagrange equations, mass matrix, gravity vector
//! - Double pendulum (2-DOF): full manipulator equation M(q)q̈ + C(q,q̇)q̇ + g(q) = τ
//! - Mass matrix symmetry check
//! - Numerical evaluation at specific configurations
//!
//! Run with: cargo run --example dynamics
use symplex::dynamics::*;
use symplex::prelude::*;
fn main() {
println!("=== Lagrangian Dynamics ===\n");
// ════════════════════════════════════════════════════════════════
// Part 1: Simple Pendulum (1-DOF)
// ════════════════════════════════════════════════════════════════
println!("--- Simple Pendulum (1-DOF) ---\n");
let ctx = Context::new();
symplex::syms!(ctx; q, qd, qdd);
let m = ctx.symbol("m");
let l = ctx.symbol("L");
let g = ctx.symbol("g");
// Simple pendulum: T = ½·m·L²·q̇², V = -m·g·L·cos(q)
//
// ctx.rational(1, 2) returns the exact rational 1/2, avoiding any
// floating-point approximation in the kinetic energy expression.
let half = ctx.rational(1, 2);
let ke = &half * &m * &l.powi(2) * &qd.powi(2);
let neg_m = -&m;
let pe = &neg_m * &g * &l * &q.cos();
println!("T = {ke}");
println!("V = {pe}");
// Euler-Lagrange equations: d/dt(∂L/∂q̇) - ∂L/∂q = τ
// Each generalized coordinate carries its own velocity and acceleration.
let coords = [GeneralizedCoordinate {
q: &q,
q_dot: &qd,
q_ddot: &qdd,
}];
let eqs = euler_lagrange(&ke, &pe, &coords);
println!("\nEquation of motion:");
println!(" τ = {}", eqs[0]);
// Mass matrix: M_ij = ∂²T / ∂q̇ᵢ∂q̇ⱼ
let mm = mass_matrix(&ke, &[&qd]).unwrap();
println!("\nMass matrix: {}", mm.get(0, 0));
// Gravity vector: gᵢ = ∂V/∂qᵢ
let gv = gravity_vector(&pe, &[&q]);
println!("Gravity: {}", gv[0]);
// Numerical evaluation at rest with unit acceleration
// m=1, L=1, g=10, q=0 (hanging straight down), qd=0, qdd=1
//
// Why τ = 1.00:
// τ = m·L²·q̈ + m·g·L·sin(q)
// At q = 0, sin(0) = 0, so the gravity term vanishes entirely.
// Only the inertial term remains: τ = 1·1²·1 = 1.00.
let tau = eqs[0]
.eval_f64_with(&[(&m, 1), (&l, 1), (&g, 10), (&q, 0), (&qd, 0), (&qdd, 1)])
.unwrap();
println!("\nτ at rest with unit acceleration: {tau:.2}");
// Evaluate at q = π/4 (45°) — now gravity contributes
// τ = m·L²·q̈ + m·g·L·sin(π/4) = 1 + 10·sin(π/4) ≈ 1 + 7.071 = 8.071
let tau_45 = eqs[0]
.eval_f64_with(&[(&m, 1), (&l, 1), (&g, 10), (&q, 1), (&qd, 0), (&qdd, 1)])
.unwrap();
println!("τ at q≈1 rad, unit accel: {tau_45:.4}");
// ════════════════════════════════════════════════════════════════
// Part 2: Double Pendulum (2-DOF)
// ════════════════════════════════════════════════════════════════
println!("\n\n--- Double Pendulum (2-DOF) ---\n");
symplex::syms!(ctx; q1, q2, qd1, qd2, qdd1, qdd2);
let m1 = ctx.symbol("m1");
let m2 = ctx.symbol("m2");
let l1 = ctx.symbol("L1");
let l2 = ctx.symbol("L2");
// Double pendulum kinetic energy:
// T = ½·m1·L1²·q̇1²
// + ½·m2·(L1²·q̇1² + L2²·q̇2² + 2·L1·L2·q̇1·q̇2·cos(q1-q2))
//
// This is the standard form where both masses are point masses
// at the end of each link.
let ke_1 = &half * &m1 * &l1.powi(2) * &qd1.powi(2);
let ke_2_term1 = &half * &m2 * &l1.powi(2) * &qd1.powi(2);
let ke_2_term2 = &half * &m2 * &l2.powi(2) * &qd2.powi(2);
let q_diff = &q1 - &q2;
let ke_2_term3 = &m2 * &l1 * &l2 * &qd1 * &qd2 * &q_diff.cos();
let ke_double = &(&(&ke_1 + &ke_2_term1) + &ke_2_term2) + &ke_2_term3;
println!("T (double pendulum):");
println!(" {ke_double}");
// Double pendulum potential energy:
// V = -(m1+m2)·g·L1·cos(q1) - m2·g·L2·cos(q2)
let neg_m1_plus_m2 = -&(&m1 + &m2);
let pe_1 = &neg_m1_plus_m2 * &g * &l1 * &q1.cos();
let neg_m2 = -&m2;
let pe_2 = &neg_m2 * &g * &l2 * &q2.cos();
let pe_double = &pe_1 + &pe_2;
println!("\nV (double pendulum):");
println!(" {pe_double}");
// Euler-Lagrange equations
let coords_double = [
GeneralizedCoordinate {
q: &q1,
q_dot: &qd1,
q_ddot: &qdd1,
},
GeneralizedCoordinate {
q: &q2,
q_dot: &qd2,
q_ddot: &qdd2,
},
];
let eqs_double = euler_lagrange(&ke_double, &pe_double, &coords_double);
println!("\nEquation of motion (joint 1):");
println!(" τ₁ = {}", eqs_double[0]);
println!("\nEquation of motion (joint 2):");
println!(" τ₂ = {}", eqs_double[1]);
// ── Mass matrix (2×2) ──────────────────────────────────────────
let mm_double = mass_matrix(&ke_double, &[&qd1, &qd2]).unwrap();
println!("\nMass matrix M(q):");
println!(" M[0,0] = {}", mm_double.get(0, 0));
println!(" M[0,1] = {}", mm_double.get(0, 1));
println!(" M[1,0] = {}", mm_double.get(1, 0));
println!(" M[1,1] = {}", mm_double.get(1, 1));
// ── Symmetry check ─────────────────────────────────────────────
//
// The mass matrix for any physical system must be symmetric:
// M[i,j] = M[j,i]
//
// We check this by comparing the off-diagonal entries.
let is_sym = mm_double.is_symmetric();
println!("\nMass matrix symmetric? {is_sym:?}");
// ── Gravity vector ─────────────────────────────────────────────
let gv_double = gravity_vector(&pe_double, &[&q1, &q2]);
println!("\nGravity vector:");
println!(" g₁ = {}", gv_double[0]);
println!(" g₂ = {}", gv_double[1]);
// ── Coriolis matrix ────────────────────────────────────────────
let coriolis = coriolis_matrix(&mm_double, &[&q1, &q2], &[&qd1, &qd2]).unwrap();
println!("\nCoriolis matrix C(q, q̇):");
println!(" C[0,0] = {}", coriolis.get(0, 0));
println!(" C[0,1] = {}", coriolis.get(0, 1));
println!(" C[1,0] = {}", coriolis.get(1, 0));
println!(" C[1,1] = {}", coriolis.get(1, 1));
// ── Full manipulator equation via convenience function ─────────
let manip = manipulator_equation(&ke_double, &pe_double, &[&q1, &q2], &[&qd1, &qd2]).unwrap();
println!("\nFull manipulator equation: M(q)q̈ + C(q,q̇)q̇ + G(q) = τ");
println!(" M shape: {:?}", manip.mass.shape());
println!(" C shape: {:?}", manip.coriolis.shape());
println!(" G length: {}", manip.gravity.len());
// ── Christoffel symbols ────────────────────────────────────────
let christoffel = christoffel_symbols(&mm_double, &[&q1, &q2]).unwrap();
println!("\nChristoffel symbols (Γ_ijk):");
for (i, plane) in christoffel.iter().enumerate().take(2) {
for (j, row) in plane.iter().enumerate().take(2) {
for (k, gamma) in row.iter().enumerate().take(2) {
let s = format!("{gamma}");
if s != "0" {
println!(" Γ_{{{i}{j}{k}}} = {s}");
}
}
}
}
// ════════════════════════════════════════════════════════════════
// Part 3: Numerical Evaluation at Specific Configuration
// ════════════════════════════════════════════════════════════════
println!("\n\n--- Numerical Evaluation ---\n");
// Configuration: q1=0, q2=0 (both links hanging straight down)
// m1=1, m2=1, L1=1, L2=1, g=9.81
// qd1=0, qd2=0 (at rest), qdd1=1, qdd2=0
println!("Config: q=(0,0), q̇=(0,0), q̈=(1,0)");
println!("Params: m1=1, m2=1, L1=1, L2=1");
// Evaluate mass matrix numerically (using g=10 integer approximation)
let subs_no_g: &[(&symplex::prelude::Ex, i64)] =
&[(&m1, 1), (&m2, 1), (&l1, 1), (&l2, 1), (&q1, 0), (&q2, 0)];
let m00 = mm_double.get(0, 0).eval_f64_with(subs_no_g);
let m01 = mm_double.get(0, 1).eval_f64_with(subs_no_g);
let m10 = mm_double.get(1, 0).eval_f64_with(subs_no_g);
let m11 = mm_double.get(1, 1).eval_f64_with(subs_no_g);
println!("\nNumerical mass matrix at q=(0,0):");
println!(
" M = [[{:.4}, {:.4}],",
m00.unwrap_or(f64::NAN),
m01.unwrap_or(f64::NAN)
);
println!(
" [{:.4}, {:.4}]]",
m10.unwrap_or(f64::NAN),
m11.unwrap_or(f64::NAN)
);
// At q1=q2=0, cos(q1-q2) = cos(0) = 1, so:
// M[0,0] = (m1+m2)·L1² = 2
// M[0,1] = M[1,0] = m2·L1·L2·cos(0) = 1
// M[1,1] = m2·L2² = 1
// Evaluate the EOM torques at the test configuration
let tau1 = eqs_double[0].eval_f64_with(&[
(&m1, 1),
(&m2, 1),
(&l1, 1),
(&l2, 1),
(&g, 10),
(&q1, 0),
(&q2, 0),
(&qd1, 0),
(&qd2, 0),
(&qdd1, 1),
(&qdd2, 0),
]);
let tau2 = eqs_double[1].eval_f64_with(&[
(&m1, 1),
(&m2, 1),
(&l1, 1),
(&l2, 1),
(&g, 10),
(&q1, 0),
(&q2, 0),
(&qd1, 0),
(&qd2, 0),
(&qdd1, 1),
(&qdd2, 0),
]);
println!("\nTorques at test config (g=10):");
println!(" τ₁ = {:.4}", tau1.unwrap_or(f64::NAN));
println!(" τ₂ = {:.4}", tau2.unwrap_or(f64::NAN));
// At q=(0,0), qd=(0,0), qdd=(1,0):
// τ₁ = M[0,0]·qdd1 + M[0,1]·qdd2 + gravity terms
// = 2·1 + 1·0 + 0 = 2 (sin(0)=0, so gravity vanishes)
// τ₂ = M[1,0]·qdd1 + M[1,1]·qdd2 + gravity terms
// = 1·1 + 1·0 + 0 = 1
// ── Determinant of mass matrix ─────────────────────────────────
let det = mm_double.det().unwrap();
println!("\ndet(M) = {det}");
let det_val = det.eval_f64_with(subs_no_g);
println!("det(M) at q=(0,0): {:.4}", det_val.unwrap_or(f64::NAN));
println!(" (Positive definite mass matrix has positive determinant)");
// ── Total time derivative ──────────────────────────────────────
println!("\n--- Total Time Derivative ---");
// d/dt(q1) = qd1
let dt_q1 = total_time_derivative(&q1, &coords_double);
let dt_q1_val = dt_q1.subs(&qd1, &ctx.int(7)).subs(&qd2, &ctx.int(0)).eval();
println!("d/dt(q1) = {dt_q1}");
println!(" at qd1=7: {dt_q1_val}");
println!("\n✓ Done!");
}