{"kind":"task","effective_mode":"full","benchmark":{"kind":"benchmark","effective_mode":"full","slug":"mmlu-pro","formal_name":"MMLU-Pro","introduction":"MMLU-Pro rebuilds MMLU with ten answer options instead of four and removes items that no longer separate models. Questions span fourteen academic and professional subjects.","introduction_ja":"","introduction_en":"","category":"Category not supplied","task_count":null,"acquisition_status":"Acquisition status not supplied","official_url":"https://huggingface.co/datasets/TIGER-Lab/MMLU-Pro","indexing_mode":"index","profile":{"resources":[],"task_format":"","scoring":"","metric":"","size":"","answer_access":"","license":"","citation":"","maintainer":"","released":"","why_hard":"","related":[],"history":"","construction":"","limitations":"","saturation":"","scores":[]}},"task_id":"a124128f-2999-51aa-bcba-7480e286ceba","task_key":"default--test--4322","task_revision_id":"1","upstream_id":"4322","short_description":"From Planck's Law, compute the Stefan - Boltzmann equation for the total density…","config":"default","split":"test","body":"{\"category\":\"chemistry\",\"options\":\"['E(T) = [(6π^5k^4T^4) / (15h^3c^3)]', 'E(T) = [(8\\\\\\\\pi^5k^5T^4) / (15h^3c^3 )]', 'E(T) = [(8\\\\\\\\pi^5k^4T^4) / (20h^3c^3 )]', 'E(T) = [(8π^4k^5T^3) / (15h^3c^3)]', 'E(T) = [(8π^5k^4T^5) / (15h^3c^3)]', 'E(T) = [(8π^5k^3T^4) / (15h^3c^3)]', 'E(T) = [(7\\\\\\\\pi^5k^4T^4) / (15h^3c^3 )]', 'E(T) = [(8\\\\\\\\pi^5k^4T^4) / (15h^3c^3 )]', 'E(T) = [(2π^5k^4T^4) / (15h^3c^3)]', 'E(T) = [(8π^5k^4T^4) / (10h^3c^3)]']\",\"question\":\"From Planck's Law, compute the Stefan - Boltzmann equation for the total density of black - body radiation as a function of temperature. That is,E (T) = ^\\\\infty\\\\int_0 E(ѵ)dѵ\",\"src\":\"stemez-PhysicalChemistry\"}","display_format":"text","language":"","answer_status":"published","assets":[],"source_url":"https://huggingface.co/datasets/TIGER-Lab/MMLU-Pro","history":"initial import","indexing_mode":"index","subproblems":[],"grids":[]}