See Greisen-Zatsepin-Kuzmin limit in All languages combined, or Wiktionary
Download JSON data for Greisen-Zatsepin-Kuzmin limit meaning in English (3.5kB)
{
"etymology_templates": [
{
"args": {
"1": "en",
"2": "limitation"
},
"expansion": "limitation",
"name": "l"
},
{
"args": {
"1": "en",
"2": "Greisen+Zatsepin+Kuzmin"
},
"expansion": "Greisen+Zatsepin+Kuzmin",
"name": "m"
}
],
"etymology_text": "From the surnames of the three physicists who proposed this limitation on long distance travel of energetic particles. From Greisen+Zatsepin+Kuzmin. Named after American physicist Kenneth Greisen, and Soviet (now Russian) physicists Georgiy Zatsepin, and Vadim Kuzmin. The Soviet team and the American each discovered the limit separately in the 1960s, being independently computed in 1966.",
"forms": [
{
"form": "the Greisen-Zatsepin-Kuzmin limit",
"tags": [
"canonical"
]
}
],
"head_templates": [
{
"args": {
"def": "1"
},
"expansion": "the Greisen-Zatsepin-Kuzmin limit",
"name": "en-prop"
}
],
"lang": "English",
"lang_code": "en",
"pos": "name",
"senses": [
{
"categories": [
{
"kind": "other",
"name": "English entries with incorrect language header",
"parents": [
"Entries with incorrect language header",
"Entry maintenance"
],
"source": "w"
},
{
"kind": "topical",
"langcode": "en",
"name": "Astronomy",
"orig": "en:Astronomy",
"parents": [
"Sciences",
"Space",
"All topics",
"Nature",
"Fundamental"
],
"source": "w"
},
{
"kind": "topical",
"langcode": "en",
"name": "Physics",
"orig": "en:Physics",
"parents": [
"Sciences",
"All topics",
"Fundamental"
],
"source": "w"
}
],
"coordinate_terms": [
{
"raw_tags": [
"of particles over this limit"
],
"tags": [
"class"
],
"word": "EECR"
},
{
"english": "the most energetic EECR discovered so far",
"word": "OMG particle"
},
{
"english": "placeholder name for that which accelerates particles above this limit",
"word": "zevatron"
}
],
"glosses": [
"A theoretical upper limit on the energy of cosmic ray protons travelling from other galaxies through the intergalactic medium to our galaxy: it is 5×10¹⁹ eV, or about 8 joules (the energy of a proton travelling at ≈ 99.99999999999999999998% the speed of light)."
],
"id": "en-Greisen-Zatsepin-Kuzmin_limit-en-name-iljPyQED",
"links": [
[
"astronomy",
"astronomy"
],
[
"physics",
"physics"
],
[
"energy",
"energy"
],
[
"cosmic ray",
"cosmic ray"
],
[
"proton",
"proton"
],
[
"intergalactic medium",
"intergalactic medium"
],
[
"galaxy",
"galaxy"
],
[
"joule",
"joule"
]
],
"raw_glosses": [
"(astronomy, physics) A theoretical upper limit on the energy of cosmic ray protons travelling from other galaxies through the intergalactic medium to our galaxy: it is 5×10¹⁹ eV, or about 8 joules (the energy of a proton travelling at ≈ 99.99999999999999999998% the speed of light)."
],
"related": [
{
"word": "Greisen-Zatsepin-Kuzmin"
},
{
"word": "Greisen-Zatsepin-Kuzmin horizon"
},
{
"word": "Greisen-Zatsepin-Kuzmin mechanism"
},
{
"word": "GZK"
},
{
"word": "GZK horizon"
},
{
"word": "GZK mechanism"
}
],
"synonyms": [
{
"word": "GZK"
},
{
"word": "GZK Limit"
},
{
"word": "GZK limit"
},
{
"word": "Greisen-Zatsepin-Kuzmin cutoff"
},
{
"word": "Greisen-Zatsepin-Kuzmin Cut-off"
},
{
"word": "Greisen-Zatsepin-Kuzmin Cut-Off"
},
{
"word": "Greisen-Zatsepin-Kuzmin Cutoff"
},
{
"word": "Greisen-Zatsepin-Kuzmin cut-off"
},
{
"word": "Greisen-Zatsepin-Kuzmin cut off"
},
{
"word": "Greisen-Zatsepin-Kuzmin Cut Off"
},
{
"word": "GZK cutoff"
},
{
"word": "GZK Cut-off"
},
{
"word": "GZK Cut-Off"
},
{
"word": "GZK Cutoff"
},
{
"word": "GZK cut-off"
},
{
"word": "GZK cut off"
},
{
"word": "GZK Cut Off"
},
{
"word": "Greisen-Zatsepin-Kuzmin Limit"
}
],
"topics": [
"astronomy",
"natural-sciences",
"physical-sciences",
"physics"
],
"wikipedia": [
"en:Georgiy Zatsepin",
"en:Kenneth Greisen",
"en:Vadim Kuzmin (physicist)"
]
}
],
"word": "Greisen-Zatsepin-Kuzmin limit"
}
{
"coordinate_terms": [
{
"raw_tags": [
"of particles over this limit"
],
"tags": [
"class"
],
"word": "EECR"
},
{
"english": "the most energetic EECR discovered so far",
"word": "OMG particle"
},
{
"english": "placeholder name for that which accelerates particles above this limit",
"word": "zevatron"
}
],
"etymology_templates": [
{
"args": {
"1": "en",
"2": "limitation"
},
"expansion": "limitation",
"name": "l"
},
{
"args": {
"1": "en",
"2": "Greisen+Zatsepin+Kuzmin"
},
"expansion": "Greisen+Zatsepin+Kuzmin",
"name": "m"
}
],
"etymology_text": "From the surnames of the three physicists who proposed this limitation on long distance travel of energetic particles. From Greisen+Zatsepin+Kuzmin. Named after American physicist Kenneth Greisen, and Soviet (now Russian) physicists Georgiy Zatsepin, and Vadim Kuzmin. The Soviet team and the American each discovered the limit separately in the 1960s, being independently computed in 1966.",
"forms": [
{
"form": "the Greisen-Zatsepin-Kuzmin limit",
"tags": [
"canonical"
]
}
],
"head_templates": [
{
"args": {
"def": "1"
},
"expansion": "the Greisen-Zatsepin-Kuzmin limit",
"name": "en-prop"
}
],
"lang": "English",
"lang_code": "en",
"pos": "name",
"related": [
{
"word": "Greisen-Zatsepin-Kuzmin"
},
{
"word": "Greisen-Zatsepin-Kuzmin horizon"
},
{
"word": "Greisen-Zatsepin-Kuzmin mechanism"
},
{
"word": "GZK"
},
{
"word": "GZK horizon"
},
{
"word": "GZK mechanism"
}
],
"senses": [
{
"categories": [
"English entries with incorrect language header",
"English eponyms",
"English lemmas",
"English multiword terms",
"English proper nouns",
"English uncountable nouns",
"en:Astronomy",
"en:Physics"
],
"glosses": [
"A theoretical upper limit on the energy of cosmic ray protons travelling from other galaxies through the intergalactic medium to our galaxy: it is 5×10¹⁹ eV, or about 8 joules (the energy of a proton travelling at ≈ 99.99999999999999999998% the speed of light)."
],
"links": [
[
"astronomy",
"astronomy"
],
[
"physics",
"physics"
],
[
"energy",
"energy"
],
[
"cosmic ray",
"cosmic ray"
],
[
"proton",
"proton"
],
[
"intergalactic medium",
"intergalactic medium"
],
[
"galaxy",
"galaxy"
],
[
"joule",
"joule"
]
],
"raw_glosses": [
"(astronomy, physics) A theoretical upper limit on the energy of cosmic ray protons travelling from other galaxies through the intergalactic medium to our galaxy: it is 5×10¹⁹ eV, or about 8 joules (the energy of a proton travelling at ≈ 99.99999999999999999998% the speed of light)."
],
"topics": [
"astronomy",
"natural-sciences",
"physical-sciences",
"physics"
],
"wikipedia": [
"en:Georgiy Zatsepin",
"en:Kenneth Greisen",
"en:Vadim Kuzmin (physicist)"
]
}
],
"synonyms": [
{
"word": "GZK"
},
{
"word": "GZK Limit"
},
{
"word": "GZK limit"
},
{
"word": "Greisen-Zatsepin-Kuzmin cutoff"
},
{
"word": "Greisen-Zatsepin-Kuzmin Cut-off"
},
{
"word": "Greisen-Zatsepin-Kuzmin Cut-Off"
},
{
"word": "Greisen-Zatsepin-Kuzmin Cutoff"
},
{
"word": "Greisen-Zatsepin-Kuzmin cut-off"
},
{
"word": "Greisen-Zatsepin-Kuzmin cut off"
},
{
"word": "Greisen-Zatsepin-Kuzmin Cut Off"
},
{
"word": "GZK cutoff"
},
{
"word": "GZK Cut-off"
},
{
"word": "GZK Cut-Off"
},
{
"word": "GZK Cutoff"
},
{
"word": "GZK cut-off"
},
{
"word": "GZK cut off"
},
{
"word": "GZK Cut Off"
},
{
"word": "Greisen-Zatsepin-Kuzmin Limit"
}
],
"word": "Greisen-Zatsepin-Kuzmin limit"
}
This page is a part of the kaikki.org machine-readable English dictionary. This dictionary is based on structured data extracted on 2024-05-06 from the enwiktionary dump dated 2024-05-02 using wiktextract (f4fd8c9 and c9440ce). The data shown on this site has been post-processed and various details (e.g., extra categories) removed, some information disambiguated, and additional data merged from other sources. See the raw data download page for the unprocessed wiktextract data.
If you use this data in academic research, please cite Tatu Ylonen: Wiktextract: Wiktionary as Machine-Readable Structured Data, Proceedings of the 13th Conference on Language Resources and Evaluation (LREC), pp. 1317-1325, Marseille, 20-25 June 2022. Linking to the relevant page(s) under https://kaikki.org would also be greatly appreciated.