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Adding Evaluation Results (#2)

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- Adding Evaluation Results (99b701c9c9339df4cd819d0df660f2b9fc88a6b5)


Co-authored-by: Open LLM Leaderboard PR Bot <leaderboard-pr-bot@users.noreply.huggingface.co>

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  1. README.md +21 -7
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  ---
 
 
 
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  tags:
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  - physics
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  - cosmology
 
 
 
 
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  model-index:
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  - name: cosmosage_qa
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  results: []
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- license: mit
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- language:
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- - en
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- pipeline_tag: text-generation
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- base_model: mistralai/Mistral-7B-v0.1
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- datasets:
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- - teknium/OpenHermes-2.5
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  ---
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  # cosmosage
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  > If matter-radiation equality occurs later in the history of the universe, then the photons spend more time in the diffusive state, which results in more damping of the CMB power spectrum. This is because the longer the photons spend in the diffusive state, the more time they have to lose energy through scattering with free electrons. Conversely, if matter-radiation equality occurs earlier in the history of the universe, then the photons spend less time in the diffusive state, which results in less damping of the CMB power spectrum.
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  >
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  > In summary, the time of matter-radiation equality affects the damping tail of the CMB power spectrum by influencing the amount of time that photons spend in the diffusive state before they are able to decouple from the matter and travel freely through the universe. The longer the photons spend in the diffusive state, the more damping occurs, and the earlier matter-radiation equality occurs, the less damping occurs.>
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
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  ---
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+ language:
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+ - en
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+ license: mit
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  tags:
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  - physics
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  - cosmology
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+ datasets:
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+ - teknium/OpenHermes-2.5
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+ pipeline_tag: text-generation
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+ base_model: mistralai/Mistral-7B-v0.1
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  model-index:
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  - name: cosmosage_qa
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  results: []
 
 
 
 
 
 
 
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  ---
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  # cosmosage
 
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  > If matter-radiation equality occurs later in the history of the universe, then the photons spend more time in the diffusive state, which results in more damping of the CMB power spectrum. This is because the longer the photons spend in the diffusive state, the more time they have to lose energy through scattering with free electrons. Conversely, if matter-radiation equality occurs earlier in the history of the universe, then the photons spend less time in the diffusive state, which results in less damping of the CMB power spectrum.
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  >
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  > In summary, the time of matter-radiation equality affects the damping tail of the CMB power spectrum by influencing the amount of time that photons spend in the diffusive state before they are able to decouple from the matter and travel freely through the universe. The longer the photons spend in the diffusive state, the more damping occurs, and the earlier matter-radiation equality occurs, the less damping occurs.>
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+
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+ # [Open LLM Leaderboard Evaluation Results](https://huggingface.co/spaces/HuggingFaceH4/open_llm_leaderboard)
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+ Detailed results can be found [here](https://huggingface.co/datasets/open-llm-leaderboard/details_Tijmen2__cosmosage_v2)
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+
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+ | Metric |Value|
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+ |---------------------------------|----:|
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+ |Avg. |60.66|
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+ |AI2 Reasoning Challenge (25-Shot)|59.73|
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+ |HellaSwag (10-Shot) |80.90|
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+ |MMLU (5-Shot) |59.57|
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+ |TruthfulQA (0-shot) |50.98|
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+ |Winogrande (5-shot) |75.93|
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+ |GSM8k (5-shot) |36.85|
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+