Update Automated MNLP evaluation report (2026-05-18)
Browse files- EVAL_REPORT.md +84 -5
EVAL_REPORT.md
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- **Model repo:** [`cs-552-2026-thinkinsidethebox/general_knowledge_model`](https://huggingface.co/cs-552-2026-thinkinsidethebox/general_knowledge_model)
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- **Owner(s):** group **thinkinsidethebox**
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- **Generated at:** 2026-05-
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- **Pipeline:** [mnlp-project-ci](https://github.com/eric11eca/mnlp-project-ci)
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_This PR is opened automatically by the course CI. It is **non-blocking** — you do not need to merge it. The next nightly run will refresh this file._
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@@ -12,7 +12,7 @@ _This PR is opened automatically by the course CI. It is **non-blocking** — yo
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| Benchmark | Accuracy | Status |
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|---|---:|---|
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| Math | — | not run |
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| Knowledge | 0.
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| Multilingual | — | not run |
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| Safety | — | not run |
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@@ -35,11 +35,90 @@ _Prompts are intentionally omitted to avoid revealing benchmark contents. For mu
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**Incorrect** (1 shown)
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- **reference**: `
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- **overall** (0/1 completions correct)
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- **extracted** (✗): `
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- **completion**:
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```text
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-
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```
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- **Model repo:** [`cs-552-2026-thinkinsidethebox/general_knowledge_model`](https://huggingface.co/cs-552-2026-thinkinsidethebox/general_knowledge_model)
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- **Owner(s):** group **thinkinsidethebox**
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- **Generated at:** 2026-05-18T02:30:25+00:00 (UTC)
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- **Pipeline:** [mnlp-project-ci](https://github.com/eric11eca/mnlp-project-ci)
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_This PR is opened automatically by the course CI. It is **non-blocking** — you do not need to merge it. The next nightly run will refresh this file._
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| Benchmark | Accuracy | Status |
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|---|---:|---|
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| Math | — | not run |
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| Knowledge | 0.3400 | ok |
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| Multilingual | — | not run |
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| Safety | — | not run |
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**Incorrect** (1 shown)
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- **reference**: `B`
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- **overall** (0/1 completions correct)
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- **extracted** (✗): `\text{B. 2.6 \times 10^5 \text{ GeV}}`
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- **completion**:
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```text
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**Step 1: Understand the process**
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The interaction of a high-energy γ-ray with a CMB photon is governed by the **Breit-Wigner resonance** and the **energy of the CMB photons**.
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The process:
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$$
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\gamma + \text{CMB} \rightarrow e^+ + e^-
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$$
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This process is **allowed** only when the energy of the γ-ray is greater than the energy of the CMB photons.
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---
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**Step 2: Determine the threshold energy**
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... [truncated 28 chars] ...
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e pair production process is given by:
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$$
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E_{\text{threshold}} = 2m_e c^2
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$$
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Where:
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- $m_e = 0.511 \text{ MeV}$ is the rest mass of the electron,
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- $c = 3 \times 10^8 \text{ m/s}$ is the speed of light.
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$$
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E_{\text{threshold}} = 2 \times 0.511 \text{ MeV} = 1.022 \text{ MeV}
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$$
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---
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**Step 3: Convert the energy of the CMB photons to GeV**
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The average photon energy of the CMB is:
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$$
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E_{\text{CMB}} = 10^{-3} \text{ eV}
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$$
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$$
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E_{\text{CMB}} = 10^{-3} \times 10^{-6} \text{ GeV} = 10^{-9} \text{ GeV}
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$$
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---
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**Step 4: Calculate the minimum energy of a γ-ray to initiate the process**
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The minimum energy of a γ-ray to initiate the pair production process is:
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$$
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E_{\text{min}} = E_{\text{threshold}} - E_{\text{CMB}} = 1.022 \text{ MeV} - 10^{-9} \text{ GeV}
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$$
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Convert 1.022 MeV to GeV:
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$$
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1.022 \text{ MeV} = 1.022 \times 10^3 \text{ eV} = 1.022 \times 10^{-3} \text{ GeV}
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$$
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$$
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E_{\text{min}} = 1.022 \times 10^{-3} \text{ GeV} - 10^{-9} \text{ GeV} \approx 1.022 \text{ GeV}
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$$
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---
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**Step 5: Convert the energy to the correct units and match the choices**
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$$
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E_{\text{min}} \approx 1.022 \text{ GeV}
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$$
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The closest answer is:
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$$
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\boxed{\text{B. 2.6 \times 10^5 \text{ GeV}}}
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$$
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```
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