"nuclear pasta" meaning in All languages combined

{
  "etymology_text": "From the resemblance of its phases to various types of pasta.",
  "head_templates": [
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      "args": {
        "1": "-"
      },
      "expansion": "nuclear pasta (uncountable)",
      "name": "en-noun"
    }
  ],
  "lang": "English",
  "lang_code": "en",
  "pos": "noun",
  "senses": [
    {
      "categories": [
        {
          "kind": "other",
          "name": "English entries with incorrect language header",
          "parents": [
            "Entries with incorrect language header",
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        },
        {
          "kind": "topical",
          "langcode": "en",
          "name": "Astrophysics",
          "orig": "en:Astrophysics",
          "parents": [
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            "Physics",
            "Sciences",
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        },
        {
          "kind": "topical",
          "langcode": "en",
          "name": "Neutron stars",
          "orig": "en:Neutron stars",
          "parents": [
            "Astrophysics",
            "Gravity",
            "Neutron",
            "Relativity",
            "Stars",
            "Astronomy",
            "Physics",
            "Acceleration",
            "Mechanics",
            "Nuclear physics",
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          "source": "w"
        }
      ],
      "examples": [
        {
          "text": "Watanabe, Gentaro, Iida, Kei, Sato, Katsuhiko (2000 August 11) “Thermodynamic properties of nuclear \"pasta\" in neutron star crusts”, in Nuclear Physics A, volume 676, numbers 1-4, →DOI, pages 455–473"
        },
        {
          "ref": "2018 September 24, M. E. Caplan, A. S. Schneider, C. J. Horowitz, “Elasticity of Nuclear Pasta”, in Physical Review Letters, volume 121, number 13, →DOI, retrieved 2021-08-26, page 132701",
          "text": "The elastic properties of neutron star crusts are relevant for a variety of currently observable or near-future electromagnetic and gravitational wave phenomena. These phenomena may depend on the elastic properties of nuclear pasta found in the inner crust.",
          "type": "quotation"
        },
        {
          "ref": "2013, José A. Pons, Daniele Viganò, Nanda Rea, “Too much \"pasta\" for pulsars to spin down”, in Nature Physics, volume 9, number 7, →Bibcode, →DOI, [arxiv.org arXiv] 1304.6546, pages 431–434",
          "text": "The inner crust [of a neutron star] is where the nuclear pasta phase, a novel state of matter having nucleons arranged in a variety of complex shapes, is expected to appear. In the innermost layers near the crust/core boundary, because of the large effect of the Coulomb lattice energy, cylindrical and planar geometries can occur, both as nuclei and as bubbles. These phases are collectively named nuclear pasta (by analogy to the shape of spaghetti, macaroni and lasagna).",
          "type": "quotation"
        }
      ],
      "glosses": [
        "A type of degenerate matter found within the crusts of neutron stars, where the competition between nuclear attraction and Coulomb repulsion forces of similar magnitude allows for the formation of a variety of complex structures assembled from neutrons and protons."
      ],
      "id": "en-nuclear_pasta-en-noun-AhXpHoHG",
      "links": [
        [
          "astrophysics",
          "astrophysics"
        ],
        [
          "degenerate",
          "degenerate"
        ],
        [
          "matter",
          "matter"
        ],
        [
          "crust",
          "crust"
        ],
        [
          "neutron star",
          "neutron star"
        ],
        [
          "magnitude",
          "magnitude"
        ],
        [
          "complex",
          "complex"
        ],
        [
          "structure",
          "structure"
        ],
        [
          "neutron",
          "neutron"
        ],
        [
          "proton",
          "proton"
        ]
      ],
      "raw_glosses": [
        "(astrophysics) A type of degenerate matter found within the crusts of neutron stars, where the competition between nuclear attraction and Coulomb repulsion forces of similar magnitude allows for the formation of a variety of complex structures assembled from neutrons and protons."
      ],
      "tags": [
        "uncountable"
      ],
      "topics": [
        "astrophysics"
      ],
      "wikipedia": [
        "nuclear pasta"
      ]
    }
  ],
  "word": "nuclear pasta"
}

{
  "etymology_text": "From the resemblance of its phases to various types of pasta.",
  "head_templates": [
    {
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      },
      "expansion": "nuclear pasta (uncountable)",
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    }
  ],
  "lang": "English",
  "lang_code": "en",
  "pos": "noun",
  "senses": [
    {
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        "English entries with topic categories using raw markup",
        "English lemmas",
        "English multiword terms",
        "English nouns",
        "English terms with non-redundant non-automated sortkeys",
        "English terms with quotations",
        "English uncountable nouns",
        "en:Astrophysics",
        "en:Neutron stars"
      ],
      "examples": [
        {
          "text": "Watanabe, Gentaro, Iida, Kei, Sato, Katsuhiko (2000 August 11) “Thermodynamic properties of nuclear \"pasta\" in neutron star crusts”, in Nuclear Physics A, volume 676, numbers 1-4, →DOI, pages 455–473"
        },
        {
          "ref": "2018 September 24, M. E. Caplan, A. S. Schneider, C. J. Horowitz, “Elasticity of Nuclear Pasta”, in Physical Review Letters, volume 121, number 13, →DOI, retrieved 2021-08-26, page 132701",
          "text": "The elastic properties of neutron star crusts are relevant for a variety of currently observable or near-future electromagnetic and gravitational wave phenomena. These phenomena may depend on the elastic properties of nuclear pasta found in the inner crust.",
          "type": "quotation"
        },
        {
          "ref": "2013, José A. Pons, Daniele Viganò, Nanda Rea, “Too much \"pasta\" for pulsars to spin down”, in Nature Physics, volume 9, number 7, →Bibcode, →DOI, [arxiv.org arXiv] 1304.6546, pages 431–434",
          "text": "The inner crust [of a neutron star] is where the nuclear pasta phase, a novel state of matter having nucleons arranged in a variety of complex shapes, is expected to appear. In the innermost layers near the crust/core boundary, because of the large effect of the Coulomb lattice energy, cylindrical and planar geometries can occur, both as nuclei and as bubbles. These phases are collectively named nuclear pasta (by analogy to the shape of spaghetti, macaroni and lasagna).",
          "type": "quotation"
        }
      ],
      "glosses": [
        "A type of degenerate matter found within the crusts of neutron stars, where the competition between nuclear attraction and Coulomb repulsion forces of similar magnitude allows for the formation of a variety of complex structures assembled from neutrons and protons."
      ],
      "links": [
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          "astrophysics",
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        ],
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        ],
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          "magnitude"
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          "complex",
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        ],
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          "neutron",
          "neutron"
        ],
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          "proton",
          "proton"
        ]
      ],
      "raw_glosses": [
        "(astrophysics) A type of degenerate matter found within the crusts of neutron stars, where the competition between nuclear attraction and Coulomb repulsion forces of similar magnitude allows for the formation of a variety of complex structures assembled from neutrons and protons."
      ],
      "tags": [
        "uncountable"
      ],
      "topics": [
        "astrophysics"
      ],
      "wikipedia": [
        "nuclear pasta"
      ]
    }
  ],
  "word": "nuclear pasta"
}