{
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  "updatedAt": "2026-09-15",
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  "scopeNote": "本轮当前已列15项有限研究账；M与归功份额为可修订判断。未覆盖内容和未核清的负面作用不按零处理，具体缺口见逐项说明。",
  "formula": {
    "q": "Q = 10^(M/2) − 1",
    "light": "Lᵢ = aᵢ × Qᵢ",
    "total": "L = Σ Lᵢ",
    "score": "S = 2 × log₁₀(1 + L)"
  },
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      "aReason": "海森堡40%计首篇非交换跃迁量代数、有界动力学计算及参与三人论文；Born 22%、Jordan 18%计矩阵识别、形式化和共同推进，Kramers、频率组合与定态、Thomas–Kuhn求和规则等前驱输入及未解析支持保留其余预算。",
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        {
          "label": "海森堡1925年首篇论文英译全文（译者署名承载体，未与德文原版逐式校勘）",
          "url": "https://www.neo-classical-physics.info/uploads/3/4/3/6/34363841/heisenberg_-_qm_interp_of_kin_and_mech.pdf"
        },
        {
          "label": "Heisenberg Society对1925–1927年量子力学形成的科学史重建",
          "url": "https://www.heisenberg-gesellschaft.de/3-die-entstehung-der-quantenmechanik-1925-ndash-1927.html"
        }
      ],
      "missing": "德文原刊尚未与英译逐式校勘；全部谱强系数、高阶振幅及三人论文内部协作细节仍有缺口。",
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          "actor": "马克斯·玻恩",
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        {
          "actor": "Pascual Jordan",
          "actorId": "EXT-LITERAL:Pascual Jordan",
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        {
          "actor": "克拉默斯外部色散输入池",
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          "actor": "频率组合与定态前驱输入池",
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          "actor": "Thomas–Kuhn求和规则输入池",
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        },
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          "actor": "未分配：1925年成熟链输入与支持",
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      "lightSharePercent": "29.2248"
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    {
      "title": "Heisenberg–Pauli场正则量子化",
      "year": "1929",
      "mReason": "对相互作用场实行正则量子化，并综合不变性、守恒量和场—粒子表述联系，采用M7.0；边界不含战后重整化、全部现代量子场论或所有后续应用。",
      "aReason": "海森堡32%、泡利32%计共同理论构造；Jordan、Dirac、Weyl、Fermi等前驱输入，以及出版机构和第一篇原文仍未解析的直接输入保留其余预算。",
      "sources": [
        {
          "label": "Heisenberg–Pauli 1929年第二篇场论论文英译全文（第一篇仍缺）",
          "url": "https://neo-classical-physics.info/uploads/3/0/6/5/3065888/heisenberg_and_pauli_-_qed_ii.pdf"
        },
        {
          "label": "Stanford Encyclopedia of Philosophy量子场论史条目（学术综述）",
          "url": "https://plato.stanford.edu/entries/quantum-field-theory/qft-history.html"
        }
      ],
      "missing": "第一篇原文尚未核读；两位作者的内部工作拆分及通向重整化量子场论的完整传递链仍有缺口。",
      "id": "OUT-SL0130-H07",
      "M": "7.0",
      "status": "已纳入研究估分",
      "budget": [
        {
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        {
          "actor": "沃尔夫冈·泡利",
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        {
          "actor": "Pascual Jordan",
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        {
          "actor": "保罗·狄拉克",
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        },
        {
          "actor": "赫尔曼·外尔",
          "actorId": "EXT-LITERAL:Hermann Weyl",
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        },
        {
          "actor": "恩里科·费米",
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          "type": "PREDECESSOR",
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        },
        {
          "actor": "1929年场量子化论文原刊出版机构",
          "actorId": "INSTITUTION:1929-QFT-ORIGINAL-PUBLICATION",
          "type": "INSTITUTION",
          "share": "0.02"
        },
        {
          "actor": "未分配：H07第一篇论文与其他场论输入",
          "actorId": "UNALLOCATED:H07-FIRST-PAPER-AND-OTHER-FIELD-INPUTS",
          "type": "UNALLOCATED",
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      "light": "1011.608851",
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      "lightSharePercent": "23.3798"
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    {
      "title": "不确定性关系",
      "year": "1927",
      "mReason": "该关系跨代进入全球量子科学，属于全球重大科学基础的M6尺度；它是一个基础限制关系而不是完整量子力学、整个测量诠释或跨领域文明基础设施，所以不升到M7。M取值依据结果的学科覆盖与持续作用，不依据原论文当前是否缺页。",
      "aReason": "海森堡68%计关系的原始提出和论文交付；玻尔的解释性讨论，以及玻恩、约尔丹、狄拉克等既有形式框架、出版机构和未解析前驱输入保留其余预算。",
      "sources": [
        {
          "label": "海森堡诺贝尔讲演",
          "url": "https://www.nobelprize.org/uploads/2018/06/heisenberg-lecture.pdf"
        }
      ],
      "missing": "1927年原文尚未逐页核读；后来的严格形式、广义关系和跨领域采用范围未在本候选中展开。",
      "id": "OUT-SL0130-H05",
      "M": "6.0",
      "status": "已纳入研究估分",
      "budget": [
        {
          "actor": "维尔纳·海森堡",
          "actorId": "SL-0130",
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        {
          "actor": "尼尔斯·玻尔",
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        {
          "actor": "马克斯·玻恩",
          "actorId": "EXT-LITERAL:Max Born",
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        },
        {
          "actor": "Pascual Jordan",
          "actorId": "EXT-LITERAL:Pascual Jordan",
          "type": "PREDECESSOR",
          "share": "0.03"
        },
        {
          "actor": "保罗·狄拉克",
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          "type": "PREDECESSOR",
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          "actor": "原始论文出版机构",
          "actorId": "INSTITUTION:1927-UNCERTAINTY-ORIGINAL-PUBLICATION",
          "type": "INSTITUTION",
          "share": "0.02"
        },
        {
          "actor": "尚未分配的直接贡献",
          "actorId": "UNALLOCATED:H05-UNREAD-PRIMARY-AND-FORMAL-ANTECEDENTS",
          "type": "UNALLOCATED",
          "share": "0.14"
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      ],
      "share": "0.68",
      "exactLight": "679.32",
      "light": "679.320000",
      "standaloneScore": "5.67",
      "lightSharePercent": "15.7001"
    },
    {
      "title": "核子双态与同位旋组织原则",
      "year": "1932",
      "mReason": "把质子与中子表为核子的两个状态，并在多核子波函数中引入后来称为同位旋的组织自由度，采用M6.0；不扩为中子实验发现、现代强相互作用理论或全部后续群论形式。",
      "aReason": "海森堡50%计1932年核子模型的直接构造；詹姆斯·查德威克的中子事实计15%，出版机构及尚未解析的直接核模型输入保留其余预算。",
      "sources": [
        {
          "label": "Physics Today对1932年核物理的科学史综述（非1932年原文）",
          "url": "https://physicstoday.aip.org/features/1932-a-watershed-year-in-nuclear-physics"
        }
      ],
      "missing": "1932年原文尚未逐页核读；Ivanenko、Majorana与Wigner命名和形式化的具体传递关系仍未闭合。",
      "id": "OUT-SL0130-H08",
      "M": "6.0",
      "status": "已纳入研究估分",
      "budget": [
        {
          "actor": "维尔纳·海森堡",
          "actorId": "SL-0130",
          "type": "PERSON",
          "share": "0.50"
        },
        {
          "actor": "詹姆斯·查德威克",
          "actorId": "SL-2236",
          "type": "PREDECESSOR",
          "share": "0.15"
        },
        {
          "actor": "1932年核子模型论文原刊出版机构",
          "actorId": "INSTITUTION:1932-NUCLEON-MODEL-ORIGINAL-PUBLICATION",
          "type": "INSTITUTION",
          "share": "0.02"
        },
        {
          "actor": "未分配：H08核子模型直接输入",
          "actorId": "UNALLOCATED:H08-DIRECT-NUCLEON-MODEL-INPUTS",
          "type": "UNALLOCATED",
          "share": "0.33"
        }
      ],
      "share": "0.50",
      "exactLight": "499.50",
      "light": "499.500000",
      "standaloneScore": "5.40",
      "lightSharePercent": "11.5442"
    },
    {
      "title": "Heisenberg–Euler恒定场QED有效作用",
      "year": "1936",
      "mReason": "在恒定电磁背景中给出重整化、非微扰的一回路自旋QED有效作用，并包含低能光—光散射项和弱电场真空对产生率，采用M6.0；不扩为非均匀场精确解、完整光—光QED或Schwinger后续形式。",
      "aReason": "海森堡35%、Hans Euler 35%计合著论文的直接构造；Sauter与Kockel的早期QED输入、出版机构和未解析直接输入保留其余预算。",
      "sources": [
        {
          "label": "Dunne 2004年Heisenberg–Euler有效拉格朗日综述（非1936年原文）",
          "url": "https://arxiv.org/pdf/hep-th/0406216"
        }
      ],
      "missing": "1936年原文及合著者内部拆分尚未核读；实验验证和后世采用范围仍需独立核验。",
      "id": "OUT-SL0130-H09",
      "M": "6.0",
      "status": "已纳入研究估分",
      "budget": [
        {
          "actor": "维尔纳·海森堡",
          "actorId": "SL-0130",
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        },
        {
          "actor": "汉斯·欧拉（非莱昂哈德·欧拉）",
          "actorId": "EXT-LITERAL:Hans Euler",
          "type": "PERSON",
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        },
        {
          "actor": "弗里茨·绍特尔",
          "actorId": "EXT-LITERAL:Fritz Sauter",
          "type": "PREDECESSOR",
          "share": "0.06"
        },
        {
          "actor": "伯恩哈德·科克尔",
          "actorId": "EXT-LITERAL:Bernhard Kockel",
          "type": "PREDECESSOR",
          "share": "0.04"
        },
        {
          "actor": "1936年Heisenberg–Euler论文原刊出版机构",
          "actorId": "INSTITUTION:1936-HEISENBERG-EULER-ORIGINAL-PUBLICATION",
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        },
        {
          "actor": "未分配：H09合著与早期QED直接输入",
          "actorId": "UNALLOCATED:H09-DIRECT-COAUTHOR-AND-EARLY-QED-INPUTS",
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      "exactLight": "349.65",
      "light": "349.650000",
      "standaloneScore": "5.09",
      "lightSharePercent": "8.0809"
    },
    {
      "title": "战时S矩阵纲领",
      "year": "1942–1944",
      "mReason": "把渐近散射算符作为相对论量子理论的自主出发点，形成试图绕开状态中心与发散困难的早期S矩阵纲领，采用M5.0；不扩为成熟现代散射量子场论。",
      "aReason": "海森堡60%计战时纲领及早期形式材料的直接交付；Kramers的可证直接输入计7%，出版机构和未解析早期S矩阵输入保留其余预算。",
      "sources": [
        {
          "label": "Blum量子场论散射史研究（同行评议定稿的arXiv版本，非战时原文）",
          "url": "https://arxiv.org/pdf/2011.05908"
        }
      ],
      "missing": "1942–1944年原文仍未逐页核读；早期具体角色及通向成熟散射理论的传递链仍有缺口。",
      "id": "OUT-SL0130-H10",
      "M": "5.0",
      "status": "已纳入研究估分",
      "budget": [
        {
          "actor": "维尔纳·海森堡",
          "actorId": "SL-0130",
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          "share": "0.60"
        },
        {
          "actor": "Hendrik Kramers",
          "actorId": "EXT-LITERAL:Hendrik Kramers",
          "type": "PERSON",
          "share": "0.07"
        },
        {
          "actor": "1942–1944年S矩阵论文原刊出版机构",
          "actorId": "INSTITUTION:1942-1944-SMATRIX-ORIGINAL-PUBLICATION",
          "type": "INSTITUTION",
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        },
        {
          "actor": "未分配：H10早期S矩阵直接输入",
          "actorId": "UNALLOCATED:H10-DIRECT-EARLY-SMATRIX-INPUTS",
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    {
      "title": "铁磁交换理论与Heisenberg模型谱系",
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      "sources": [
        {
          "label": "海森堡1928年铁磁理论论文英译全文（非德文原版）",
          "url": "https://neo-classical-physics.info/uploads/3/0/6/5/3065888/heisenberg_-_on_the_theory_of_ferromagnetism.pdf"
        },
        {
          "label": "2007年数值微磁学综述：交换能与1928年理论的来源桥梁",
          "url": "https://web.math.ucsb.edu/~cgarcia/Papers/Garcia-Cervera_ReviewSEMA.pdf"
        },
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          "label": "2020年二维磁性材料论文：Heisenberg模型的实际复用及量子修正边界",
          "url": "https://arxiv.org/pdf/1912.05230"
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      ],
      "missing": "持续采用的完整范围、材料适用边界及M5与M6的节点比较仍待更系统核验。",
      "id": "OUT-SL0130-H06",
      "M": "5.0",
      "status": "已纳入研究估分",
      "budget": [
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          "actor": "维尔纳·海森堡",
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        {
          "actor": "弗里茨·伦敦",
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        {
          "actor": "皮埃尔·外斯",
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          "actor": "沃尔夫冈·泡利",
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        {
          "actor": "尤金·维格纳",
          "actorId": "EXT-LITERAL:Eugene Wigner",
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        },
        {
          "actor": "弗里德里希·洪德",
          "actorId": "EXT-LITERAL:Friedrich Hund",
          "type": "PREDECESSOR",
          "share": "0.03"
        },
        {
          "actor": "阿诺德·索末菲",
          "actorId": "EXT-LITERAL:Arnold Sommerfeld",
          "type": "PREDECESSOR",
          "share": "0.02"
        },
        {
          "actor": "1928年铁磁理论论文出版机构",
          "actorId": "INSTITUTION:1928-FERROMAGNETISM-PUBLICATION",
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        },
        {
          "actor": "未分配：H06其他磁学与材料输入",
          "actorId": "UNALLOCATED:H06-OTHER-MAGNETISM-AND-MATERIAL-INPUTS",
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    {
      "title": "克拉默斯—海森堡色散公式",
      "year": "1925",
      "mReason": "取M4.5：它是进入国际研究与持续命名使用的重要理论方法，Raman本人同代讨论证明这条路径进入实际问题解释；但Raman明确当时结构和定量认识不足，原论文正文亦未核读，故不升为完整领域改变或散射理论底座。",
      "aReason": "海森堡30%、Kramers 45%计联合公式；经典色散与旧量子论、外部色散输入和出版支持保留其余预算。",
      "sources": [
        {
          "label": "拉曼1930年诺贝尔讲演",
          "url": "https://www.nobelprize.org/uploads/2018/06/raman-lecture.pdf"
        }
      ],
      "missing": "1925年原论文正文、两位作者的内部拆分及公式到Raman问题的完整传递链仍未闭合。",
      "id": "OUT-SL0130-H03-KRAMERS-HEISENBERG-DISPERSION",
      "M": "4.5",
      "status": "已纳入研究估分",
      "budget": [
        {
          "actor": "亨德里克·克拉默斯",
          "actorId": "EXT-LITERAL:Hendrik Anthony Kramers",
          "type": "PERSON",
          "share": "0.55"
        },
        {
          "actor": "维尔纳·海森堡",
          "actorId": "SL-0130",
          "type": "PERSON",
          "share": "0.30"
        },
        {
          "actor": "尼尔斯·玻尔",
          "actorId": "SL-0019",
          "type": "PREDECESSOR",
          "share": "0.10"
        },
        {
          "actor": "尚未分配的直接贡献",
          "actorId": "EXT-LITERAL:unresolved classical-dispersion and old-quantum inputs",
          "type": "UNALLOCATED",
          "share": "0.05"
        }
      ],
      "share": "0.30",
      "exactLight": "53.04838230116768403676263585578054534207371579206766074035492168328905644618481414700901197836106465",
      "light": "53.048382",
      "standaloneScore": "3.47",
      "lightSharePercent": "1.2260"
    },
    {
      "title": "氦原子谱的交换对称处理",
      "year": "1926",
      "mReason": "完整结果形成了被同行接受并获随后实验支持的多电子原子交换处理，达到广泛专业方法/重要科学结果的M4尺度。它不是完整量子统计、全部原子结构或后世交换力理论，因此不升至全球学科基础的M6–M7。份额与模型假设局限属于a和边界，不在M重复扣减。",
      "aReason": "海森堡45%计两篇共振与二电子论文的直接建模和交付；泡利、玻恩、玻色、爱因斯坦的构成性前史、出版机构和未解析直接输入保留其余预算。",
      "sources": [
        {
          "label": "Heisenberg 1926氦原子研究的学术重建",
          "url": "https://link.springer.com/article/10.1140/epjh/s13129-026-00127-z"
        }
      ],
      "missing": "两篇1926年原文尚未逐页核读；与氢的正、仲态类比及更广的后世接受仍待正文级核验。",
      "id": "OUT-SL0130-H04",
      "M": "4.0",
      "status": "已纳入研究估分",
      "budget": [
        {
          "actor": "维尔纳·海森堡",
          "actorId": "SL-0130",
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        },
        {
          "actor": "沃尔夫冈·泡利",
          "actorId": "SL-0815",
          "type": "PREDECESSOR",
          "share": "0.10"
        },
        {
          "actor": "马克斯·玻恩",
          "actorId": "EXT-LITERAL:Max Born",
          "type": "PREDECESSOR",
          "share": "0.03"
        },
        {
          "actor": "萨特延德拉·纳特·玻色",
          "actorId": "EXT-LITERAL:Satyendra Nath Bose",
          "type": "PREDECESSOR",
          "share": "0.04"
        },
        {
          "actor": "阿尔伯特·爱因斯坦",
          "actorId": "SL-0001",
          "type": "PREDECESSOR",
          "share": "0.04"
        },
        {
          "actor": "原始论文出版机构",
          "actorId": "INSTITUTION:1926-HELIUM-PAPERS-ORIGINAL-PUBLICATION",
          "type": "INSTITUTION",
          "share": "0.02"
        },
        {
          "actor": "尚未分配的直接贡献",
          "actorId": "UNALLOCATED:H04-DIRECT-ATOMIC-AND-EXCHANGE-INPUTS",
          "type": "UNALLOCATED",
          "share": "0.32"
        }
      ],
      "share": "0.45",
      "exactLight": "44.55",
      "light": "44.550000",
      "standaloneScore": "3.32",
      "lightSharePercent": "1.0296"
    },
    {
      "title": "高能总截面对数平方增长预言",
      "year": "1952",
      "mReason": "激波模型给出高能强子总截面可按对数平方随能量增长的早期预言，后来ISR观察到总截面上升，采用M3.0；不扩为ISR实验、Cheng–Wu模型、完整渐近证明或模型其他细节。",
      "aReason": "海森堡60%计1952年预测的直接推导与交付；出版机构、1952年前高能输入及内部推导和传播的未解析部分保留其余预算。",
      "sources": [
        {
          "label": "Amaldi对ISR总截面结果的参与者回忆（含1952年原刊引用，非原文）",
          "url": "https://arxiv.org/pdf/1206.3954"
        }
      ],
      "missing": "1952年原文尚未核读；部分文献写1954年的日期差异、模型全貌和后世接收链仍待核验。",
      "id": "OUT-SL0130-H11",
      "M": "3.0",
      "status": "已纳入研究估分",
      "budget": [
        {
          "actor": "维尔纳·海森堡",
          "actorId": "SL-0130",
          "type": "PERSON",
          "share": "0.60"
        },
        {
          "actor": "1952年截面增长论文原刊出版机构",
          "actorId": "INSTITUTION:1952-CROSS-SECTION-ORIGINAL-PUBLICATION",
          "type": "INSTITUTION",
          "share": "0.04"
        },
        {
          "actor": "未分配：H11在1952年前的高能输入",
          "actorId": "UNALLOCATED:H11-PRE-1952-HIGH-ENERGY-INPUTS",
          "type": "UNALLOCATED",
          "share": "0.16"
        },
        {
          "actor": "未分配：H11内部推导与传播",
          "actorId": "UNALLOCATED:H11-INTERNAL-DERIVATION-AND-TRANSMISSION",
          "type": "UNALLOCATED",
          "share": "0.20"
        }
      ],
      "share": "0.60",
      "exactLight": "18.37366596101027599199336126659631120231733083595130096114502911675556663183542932806548865027580177",
      "light": "18.373666",
      "standaloneScore": "2.57",
      "lightSharePercent": "0.4246"
    },
    {
      "title": "均匀各向同性湍流的受限统计模型",
      "year": "1948",
      "mReason": "以含波数相关项的耗散表达处理均匀各向同性湍流谱，纳入低雷诺数频率成分并提出逆七次方谱，采用M3.0；这是受限专业模型，不是湍流普适解。",
      "aReason": "海森堡55%计1948年模型、表达和论文交付；出版机构及未解析的直接湍流输入保留其余预算。",
      "sources": [
        {
          "label": "2024年早期各向同性湍流同行评议综述（非1948年原文）",
          "url": "https://www.mdpi.com/2073-4433/15/4/494"
        }
      ],
      "missing": "1948年原文、模型的引用与采用范围及直接前驱输入仍需正文级核验。",
      "id": "OUT-SL0130-H12-ISOTROPIC-TURBULENCE-1948",
      "M": "3.0",
      "status": "已纳入研究估分",
      "budget": [
        {
          "actor": "维尔纳·海森堡",
          "actorId": "SL-0130",
          "type": "PERSON",
          "share": "0.55"
        },
        {
          "actor": "未分配：1948年湍流模型直接输入",
          "actorId": "H12_UNRESOLVED_DIRECT_INPUTS",
          "type": "UNALLOCATED",
          "share": "0.45"
        }
      ],
      "share": "0.55",
      "exactLight": "16.84252713092608632599391449437995193545755326628869254771627669035926941251581021739336459608615162",
      "light": "16.842527",
      "standaloneScore": "2.50",
      "lightSharePercent": "0.3893"
    },
    {
      "title": "德国参与CERN筹建及早期科学政策工作",
      "year": "1951–1957",
      "mReason": "现有材料支持德国代表参与1951年早期决议、德国成为正式创始成员并提供经费，以及海森堡1954–1957年处于科学政策委员会主席位置，采用M3.5；不扩为完整CERN平台或后来实验设施成果。",
      "aReason": "海森堡25%只计现有材料可界定的个人参与；德意志联邦共和国45%、UNESCO与CERN筹备机构15%，尚未解析的德国代表团和早期政策共同者保留15%。",
      "sources": [
        {
          "label": "马克斯·普朗克物理研究所机构史：德国参与CERN的具体行动",
          "url": "https://www.mpp.mpg.de/en/about-us/history"
        },
        {
          "label": "CERN科学政策委员会历任主席官方名录",
          "url": "https://council.web.cern.ch/en/content/chairs-scientific-policy-committee"
        }
      ],
      "missing": "1951年会议和资金安排的完整正文、主席任内具体政策建议及其他参与者的个人贡献仍未闭合；主席名录只证明任职。",
      "id": "OUT-SL0130-H14-CERN-GERMAN-PARTICIPATION-AND-EARLY-SCIENTIFIC-POLICY",
      "M": "3.5",
      "status": "已纳入研究估分",
      "budget": [
        {
          "actor": "维尔纳·海森堡",
          "actorId": "SL-0130",
          "type": "PERSON",
          "share": "0.25"
        },
        {
          "actor": "德意志联邦共和国",
          "actorId": "EXT-LITERAL:Federal Republic of Germany",
          "type": "INSTITUTION",
          "share": "0.45"
        },
        {
          "actor": "联合国教科文组织与CERN筹备机构",
          "actorId": "EXT-LITERAL:UNESCO and CERN preparatory institutions",
          "type": "INSTITUTION",
          "share": "0.15"
        },
        {
          "actor": "未分配：德国代表团与早期政策共同者",
          "actorId": "EXT-LITERAL:unresolved German and early-policy contributors",
          "type": "UNALLOCATED",
          "share": "0.15"
        }
      ],
      "share": "0.25",
      "exactLight": "13.80853312975872700987377599441203078670627607746729160204223559339708921607657122264644961315550765",
      "light": "13.808533",
      "standaloneScore": "2.34",
      "lightSharePercent": "0.3191"
    },
    {
      "title": "宇宙线硬成分的寿命解释",
      "year": "1938",
      "mReason": "以不稳定穿透粒子约2微秒的静止寿命，定量解释宇宙线硬成分在空气与致密物质中的吸收差异，采用M3.0；不扩为粒子实验发现、完整现代身份、产生机制或后来的测量。",
      "aReason": "海森堡40%、Hans Euler 40%计合著解释；原刊机构2%，未解析的直接宇宙线输入保留18%。同期评论用于事实与接收核验，不领取原始论文份额。",
      "sources": [
        {
          "label": "Blackett 1938年Nature同期评论公开摘要/预览（付费全文未读）",
          "url": "https://www.nature.com/articles/142992a0"
        },
        {
          "label": "Rossi 1938年Nature同期评论公开摘要/预览（付费全文未读）",
          "url": "https://www.nature.com/articles/142993a0"
        }
      ],
      "missing": "合著原文尚未核读；Kulenkampff、Bhabha等实验和理论输入，以及后来的接收与校正范围仍有缺口。",
      "id": "OUT-SL0130-H13",
      "M": "3.0",
      "status": "已纳入研究估分",
      "budget": [
        {
          "actor": "维尔纳·海森堡",
          "actorId": "SL-0130",
          "type": "PERSON",
          "share": "0.40"
        },
        {
          "actor": "汉斯·欧拉（非莱昂哈德·欧拉）",
          "actorId": "EXT-LITERAL:Hans Euler",
          "type": "PERSON",
          "share": "0.40"
        },
        {
          "actor": "1938年宇宙线寿命论文原刊出版机构",
          "actorId": "INSTITUTION:1938-COSMIC-RAY-LIFETIME-ORIGINAL-PUBLICATION",
          "type": "INSTITUTION",
          "share": "0.02"
        },
        {
          "actor": "未分配：H13宇宙线直接输入",
          "actorId": "UNALLOCATED:H13-DIRECT-COSMIC-RAY-INPUTS",
          "type": "UNALLOCATED",
          "share": "0.18"
        }
      ],
      "share": "0.40",
      "exactLight": "12.24911064067351732799557417773087413487822055730086730743001941117037775455695288537699243351720118",
      "light": "12.249111",
      "standaloneScore": "2.24",
      "lightSharePercent": "0.2831"
    },
    {
      "title": "互补性：观测条件与波粒描述的解释框架",
      "year": "1927–1928",
      "mReason": "七节公开框架组织观测、定义与既有波粒描述；仍有争议，未主张唯一正确解。",
      "aReason": "沿用既有完整预算；海森堡4%只计与互补性框架直接相连的讨论输入，玻尔的综合、其他贡献者、出版机构和未分配部分全部保留，本轮未重裁。",
      "sources": [
        {
          "label": "Bohr 1928原始概念论证文本（Gutenberg缓存）",
          "url": "https://www.gutenberg.org/files/72800/72800-h/72800-h.htm"
        },
        {
          "label": "Niels Bohr Institute机构史（公共表述与科学讨论范围）",
          "url": "https://nbi.ku.dk/english/www/institute/history/the_copenhagen_interpretation"
        }
      ],
      "missing": "沿用原采用结果；本轮未重审完整原刊、争议范围或完整预算。",
      "id": "OUT-SL0019-1927-1928-COMPLEMENTARITY-FRAMEWORK",
      "M": "4.9",
      "status": "已纳入研究估分",
      "budget": [
        {
          "actor": "尼尔斯·玻尔",
          "actorId": "SL-0019",
          "type": "PERSON",
          "share": "0.65"
        },
        {
          "actor": "维尔纳·海森堡",
          "actorId": "SL-0130",
          "type": "PERSON",
          "share": "0.04"
        },
        {
          "actor": "保罗·狄拉克",
          "actorId": "SL-0021",
          "type": "PERSON",
          "share": "0.025"
        },
        {
          "actor": "Pascual Jordan",
          "actorId": "EXT-LITERAL:Pascual Jordan",
          "type": "PERSON",
          "share": "0.02"
        },
        {
          "actor": "埃尔温·薛定谔",
          "actorId": "SL-0061",
          "type": "PERSON",
          "share": "0.035"
        },
        {
          "actor": "马克斯·玻恩",
          "actorId": "EXT-LITERAL:Max Born",
          "type": "PERSON",
          "share": "0.03"
        },
        {
          "actor": "阿尔伯特·爱因斯坦",
          "actorId": "SL-0001",
          "type": "PERSON",
          "share": "0.03"
        },
        {
          "actor": "Louis de Broglie",
          "actorId": "EXT-LITERAL:Louis de Broglie",
          "type": "PERSON",
          "share": "0.03"
        },
        {
          "actor": "OTHER CONSTITUTIVE QUANTUM ANTECEDENTS",
          "actorId": "POOL:OTHER_CONSTITUTIVE_QUANTUM_ANTECEDENTS",
          "type": "PREDECESSOR",
          "share": "0.035"
        },
        {
          "actor": "PUBLICATION LECTURE INSTITUTION",
          "actorId": "POOL:PUBLICATION_LECTURE_INSTITUTION",
          "type": "INSTITUTION",
          "share": "0.02"
        },
        {
          "actor": "未分配",
          "actorId": "POOL:UNALLOCATED_W2",
          "type": "UNALLOCATED",
          "share": "0.085"
        }
      ],
      "share": "0.04",
      "exactLight": "11.23353172505781527640769479662044287473217433508381601176421623889311351254741676812206109493524409",
      "light": "11.233532",
      "standaloneScore": "2.18",
      "lightSharePercent": "0.2596"
    },
    {
      "title": "《Physics and Philosophy》大众讲演与哲学文本",
      "year": "1955–1958",
      "mReason": "Gifford讲演及1958年大众文本面向非专业读者解释现代物理的哲学与可能社会含义，并比较古希腊原子论、数学形式和现代粒子转化，同时明确统一粒子动力学尚未解决，采用M2.0；哲学解释不视为已证实验事实。",
      "aReason": "海森堡60%计讲演和文本的直接交付；Northrop署名导言10%、Gifford讲演机构8%、原版出版机构5%，编辑、翻译及其他直接文本输入的未解析部分保留17%。",
      "sources": [
        {
          "label": "AIP收录的1958年书第71–72页节选（非全书）",
          "url": "https://history.aip.org/history/exhibits/heisenberg/physics-and-philosophy.html"
        },
        {
          "label": "F. S. C. Northrop署名导言（目标读者与内容定位）",
          "url": "https://giffordarchives.org/books/physics-and-philosophy/introduction"
        },
        {
          "label": "St Andrews Gifford Lectures官方名录（1955–1956年讲演）",
          "url": "https://gifford.wp.st-andrews.ac.uk/the-st-andrews-gifford-lectures-from-1889-to-the-present/"
        }
      ],
      "missing": "全书、读者接收与教育影响仍未系统核验；1930年专业教材和其他著作仍是独立缺口。",
      "id": "OUT-SL0130-H17b",
      "M": "2.0",
      "status": "已纳入研究估分",
      "budget": [
        {
          "actor": "维尔纳·海森堡",
          "actorId": "SL-0130",
          "type": "PERSON",
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        },
        {
          "actor": "F. S. C. 诺思罗普",
          "actorId": "EXT-LITERAL:F. S. C. Northrop",
          "type": "PERSON",
          "share": "0.10"
        },
        {
          "actor": "圣安德鲁斯大学Gifford讲演机构（1955–1956）",
          "actorId": "INSTITUTION:UNIVERSITY-OF-ST-ANDREWS-GIFFORD-LECTURES-1955-1956",
          "type": "INSTITUTION",
          "share": "0.08"
        },
        {
          "actor": "1958年《Physics and Philosophy》原版出版机构",
          "actorId": "INSTITUTION:1958-PHYSICS-PHILOSOPHY-ORIGINAL-PUBLICATION",
          "type": "INSTITUTION",
          "share": "0.05"
        },
        {
          "actor": "未分配：H17b编辑、翻译与直接文本输入",
          "actorId": "UNALLOCATED:H17B-EDITORIAL-TRANSLATION-AND-DIRECT-TEXT-INPUTS",
          "type": "UNALLOCATED",
          "share": "0.17"
        }
      ],
      "share": "0.60",
      "exactLight": "5.40",
      "light": "5.400000",
      "standaloneScore": "1.61",
      "lightSharePercent": "0.1248"
    }
  ],
  "exclusions": [
    {
      "id": "H15",
      "title": "MPP研究能力与人才培养",
      "reason": "MPP官方历史支持Heisenberg在1955年作出研究方向转移，并记录其任内后来设立等离子体研究所；但现有材料没有冻结具体资源、共同决策者、人才培养动作、可观察科研能力终端或反事实连接。职衔、方向决定和团队后来所有发现都不能自动记作个人科研成果，因此目前既不计分也不填0。"
    },
    {
      "id": "H18",
      "title": "晚期统一理论与对称破缺",
      "reason": "Nobel官方传记只说明1953年后工作重心转向基本粒子统一场理论，现有队列也明确不能把未达成统一理论包装为成功。当前没有具体被证明、被采用或可与失败纲领分离的对称破缺结果，因此不能以研究方向、论文数量或声望发光；同时尚未完成对可能独立概念的检索，故延期而非填0。"
    },
    {
      "id": "H19",
      "title": "战争时期研究、文化代表与个体帮助",
      "reason": "AIP材料支持1939年报告、莱比锡反应堆小组领导、柏林研究和行政联系等行动，也明确德国项目截至战争结束未达到链式反应；Farm Hall只证明战后谈话和相互冲突的动机解释。研究参与不能写成成功造堆，未造弹不能写成已证道德抵制，文化出访或帮助同行也没有逐案结果证据。正向成果、可分离伤害和动机必须分账，现阶段均延期而不填0、不相互抵消。"
    },
    {
      "id": "H16-HUMBOLDT-EXCHANGE-FUNDING",
      "title": "H16-HUMBOLDT-EXCHANGE-FUNDING",
      "reason": "现有材料只证明SL-0130为首任主席，不能把未准入写成实际贡献份额0，也不能从头衔推定正份额。暂不形成任何a预算。"
    },
    {
      "id": "H12-1923-STABILITY",
      "title": "H12-1923-STABILITY",
      "reason": "1923/24流体稳定性原文及独立正确结果未闭合；1948湍流不代替这一缺口。"
    },
    {
      "id": "H17a-NOBEL",
      "title": "H17a-NOBEL",
      "reason": "诺贝尔讲演的科学阐释并入已有科学成果证据，不按章节另计。"
    },
    {
      "id": "H17-OTHER-BOOKS",
      "title": "H17-OTHER-BOOKS",
      "reason": "1930专业教材及其他著作未逐项核读和去重，不能用诺奖讲演替代全部教育文化覆盖。"
    }
  ],
  "provisionalCount": 0,
  "provenance": {
    "releaseId": "research-200-20260914",
    "baselineLedgerSha256": "8bdd406b3e20ae22357644499e622922c670ff11010df0478c70c23b38902108",
    "c24DeltaSha256": "b0b96144d1d3397e54a61c3d706ff2da5920fe7617e3bef50407149cb97d9d62",
    "generatorSha256": "25de659e9852503508e7c27d8a31773b8da5d6310531b1e3699d18cc94319929"
  },
  "priorScopeNote": "15项已列贡献的研究估分。账本覆盖有限的主要成果，尚未穷尽生涯。M与归功份额是可修订的评估判断；未覆盖经历和负面影响不按零处理。",
  "rank": 8
}
