This PR implements a new strategy for simplifying `have`-telescopes in
`Sym.simp` that achieves linear kernel type-checking time instead of
quadratic.
## Problem
When simplifying deep `have`-telescopes, the previous approach using
`have_congr'` produced proofs that type-checked in quadratic time. The
simplifier itself was fast, but the kernel became the bottleneck for
large telescopes.
For example, at n=100:
- **Before**: simp = 2.4ms, kernel = **225ms**
- **After**: simp = 3.5ms, kernel = **10ms**
The quadratic behavior occurred because the kernel creates fresh free
variables for each binder when type-checking, destroying sharing and
producing O(n²) intermediate terms.
## Solution
We transform sequential `have`-telescopes into a parallel
beta-application form:
```
have x₁ := v₁; have x₂ := v₂[x₁]; b[x₁, x₂]
↓ (definitionally equal)
(fun x₁ x₂' => b[x₁, x₂' x₁]) v₁ (fun x₁ => v₂[x₁])
```
This parallel form leverages the efficient simplifier for lambdas in
`Sym.simp`. This form enables:
1. Independent simplification of each argument
2. Proof construction using standard congruence lemmas
3. Linear kernel type-checking time
The algorithm has three phases:
1. **`toBetaApp`**: Transform telescope → parallel beta-application
2. **`simpBetaApp`**: Simplify using `congr`/`congrArg`/`congrFun'` and
`simpLambda`
3. **`toHave`**: Convert back to `have` form
## Benchmark Results
### Benchmark 1: Chain with all variables used in body
| n | Before (simp) | Before (kernel) | After (simp) | After (kernel) |
|---|---------------|-----------------|--------------|----------------|
| 50 | 1.2ms | 32ms | 1.6ms | 4.4ms |
| 100 | 2.4ms | **225ms** | 3.5ms | **10ms** |
| 200 | 4.5ms | — | 8.4ms | 27ms |
| 500 | 11.7ms | — | 33.6ms | 128ms |
### Benchmark 3: Parallel declarations (simplified values)
| n | Before (simp) | Before (kernel) | After (simp) | After (kernel) |
|---|---------------|-----------------|--------------|----------------|
| 50 | 0.5ms | 24ms | 0.8ms | 1.8ms |
| 100 | 1.2ms | **169ms** | 1.8ms | **5.3ms** |
| 200 | 2.2ms | — | 3.9ms | 17ms |
| 500 | 5.9ms | — | 12.3ms | 93ms |
### Benchmark 5: Chain with single dependency
| n | Before (simp) | Before (kernel) | After (simp) | After (kernel) |
|---|---------------|-----------------|--------------|----------------|
| 100 | 1.6ms | 6.2ms | 1.8ms | 6.2ms |
| 200 | 2.8ms | 21.6ms | 4.4ms | 16.5ms |
| 500 | 7.3ms | **125ms** | 12.8ms | **72ms** |
Key observations:
- Kernel time is now **linear** in telescope depth (previously
quadratic)
- Simp time increases slightly due to the transformation overhead
- Total time (simp + kernel) is dramatically reduced for large
telescopes
- The improvement is most pronounced when the body depends on many
variables
## Trade-offs
- Proof sizes are larger (more congruence lemma applications)
- Simp time has ~1.5x overhead from the transformation
- For very small telescopes (n < 10), the overhead may not pay off
The optimization targets the critical path: kernel type-checking was the
bottleneck preventing scaling to realistic symbolic simulation
workloads.
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