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NūhouʻIke ʻia ka moho ʻeleʻele māmā māmā e LIGO

ʻIke ʻia ka moho ʻeleʻele māmā māmā e LIGO

NĀ HOʻOPIʻI: ʻO ka ʻike a me nā manaʻo i hoʻopuka hou ʻia i loko o nā ʻatikala na ka poʻe e haʻi nei iā lākou a na lākou ke kuleana. Hoolaha ma The European Times 'a'ole 'o ia ka 'ae 'ana i ka mana'o, akā 'o ke kuleana e ha'i.

NĀ UNUHI HOPE: Ua paʻi ʻia nā ʻatikala a pau ma kēia pūnaewele ma ka ʻōlelo Pelekania. Hana ʻia nā ʻano unuhi ma o ke kaʻina ʻakomi i kapa ʻia ʻo ka unuhi neural. Inā kānalua, e nānā mau i ka ʻatikala kumu. Mahalo iā ʻoe no ka hoʻomaopopo ʻana.

Nūpepa
Nūpepahttps://europeantimes.news
The European Times Manaʻo ka nūhou e uhi i nā nūhou e hoʻonui i ka ʻike o nā kamaʻāina a puni ʻEulopa.


Ma Mei 2023, ma hope koke iho o ka huli ʻana o LIGO (Laser Interferometer Gravitational-wave Observatory) no kāna ʻehā o ka nānā ʻana, ua ʻike ʻia he hōʻailona hawewe-kaumaha mai ka hui ʻana o kekahi mea, he hoku neutron paha, me ka lua eleele i manaoia he 2.5 a 4.5 ka nui ma mua o ko ka La.

ʻO kēia hōʻailona, ​​i kapa ʻia ʻo GW230529, he mea hoihoi ia i ka poʻe noiʻi no ka mea e hāʻule ana ka nui o ka lua ʻeleʻele o ka moho i loko o kahi āpau i kapa ʻia ma waena o nā hōkū neutron nui loa i ʻike ʻia, ʻoi aku ka nui ma mua o ʻelua mau pūʻulu lā, a me nā puka ʻeleʻele māmā loa i ʻike ʻia, ma kahi o ʻelima ka nui o ka lā. ʻOiai ʻaʻole hiki i ka hōʻailona nalu ʻumekaumaha wale ke hōʻike i ke ʻano maoli o kēia mea, ʻo ka ʻike ʻana o nā hanana like i ka wā e hiki mai ana, ʻoi aku ka nui o nā mea i hele pū ʻia me ka ʻā ʻana o ka mālamalama, hiki ke paʻa i ke kī e pane ai i ka nīnau pehea e hiki ai i nā puka ʻeleʻele māmā.

The image shows the coalescence and merger of a lower mass-gap black hole (dark gray surface) with a neutron star (greatly tidally deformed by the black hole's gravity). This still image from a simulation of the merger highlights just the neutron star's lower density components, ranging from 60 grams per cubic centimeter (dark blue) to 600 kilograms per cubic centimeter (white). Its shape highlights the strong deformations of the low-density material of the neutron star
Credit: Ivan Markin, Tim Dietrich (University of Potsdam), Harald Paul Pfeiffer, Alessandra Buonanno (Max Planck Institute for Gravitational Physics

Hōʻike ke kiʻi i ka hui ʻana a me ka hoʻohui ʻana o kahi lua ʻeleʻele haʻahaʻa (ka ʻeleʻele ʻeleʻele) me kahi hōkū neutron (ua hoʻololi ʻia e ka umekaumaha o ka lua ʻeleʻele). Hōʻike ʻia kēia kiʻi paʻa mai ka hoʻohālikelike hui ʻana i nā ʻāpana haʻahaʻa haʻahaʻa o ka hōkū neutron, mai ka 60 grams no ke kenimika cubic (uliuli ʻeleʻele) a i ka 600 kilokani no ke kenimika cubic (keʻokeʻo). Hōʻike kona ʻano i nā deformations ikaika o nā mea haʻahaʻa haʻahaʻa o ka hōkū neutron. Kiʻi Kiʻi: Ivan Markin, Tim Dietrich (University of Potsdam), Harald Paul Pfeiffer, Alessandra Buonanno (Max Planck Institute for Gravitational Physics

"ʻO ka ʻike hou loa e hōʻike ana i ka mana ʻepekema maikaʻi loa o ka ʻenehana ʻike hawewe-gravitational, ʻoi aku ka maʻalahi ma mua o ke kolu o ka nānā ʻana," wahi a Jenne Driggers (PhD '15), ʻepekema alakaʻi ʻike ma LIGO Hanford ma Wakinekona, ʻO kekahi o nā keʻena ʻelua, me LIGO Livingston ma Louisiana, i kūkulu ʻia ka LIGO Observatory.

LINK hana i ka mōʻaukala ma 2015 ma hope o ka hoʻokō ʻana i ka ʻike mua ʻana i nā nalu gravity ma ka lewa. Mai ia manawa, ua ʻike ʻo LIGO a me kāna hoa ʻike maka ma ʻEulopa, ʻo Virgo, ma kahi o 100 mergers ma waena o nā lua ʻeleʻele, kahi lima ma waena o nā hōkū neutron, a me nā hui pū ʻana ma waena o nā hōkū neutron a me nā lua ʻeleʻele. Ua hui pū ka mea ʻike Kepani ʻo KAGRA i ka ʻupena ʻumekaumaha ma 2019, a ʻo ka hui o nā ʻepekema nāna e hōʻuluʻulu pū i ka ʻikepili mai nā mea ʻike ʻekolu a ʻike ʻia ʻo LIGO–Virgo–KAGRA (LVK). Hāʻawi kālā ʻia nā hale nānā LIGO e ka National Science Foundation (NSF), a ua hāpai ʻia, kūkulu ʻia, a hoʻokele ʻia e Caltech a me MIT.

Hōʻike pū ka ʻike hou loa e ʻoi aku ka maʻamau o nā hui ʻana e pili ana i nā lua ʻeleʻele māmā ma mua o ka mea i manaʻo ʻia ma mua.

"ʻO kēia ʻike, ʻo ka mua o kā mākou hopena hoihoi mai ka hā o ka nānā ʻana i ka holo ʻana o LIGO–Virgo–KAGRA, e hōʻike ana he ʻoi aku ka nui o nā hui like ma waena o nā hōkū neutron a me nā lua ʻeleʻele haʻahaʻa haʻahaʻa ma mua o kā mākou i manaʻo ai ma mua," wahi a Jess McIver, he kaukaʻi kōkua ma ke Kulanui o British Columbia, hope waha ʻōlelo o ka LIGO Scientific Collaboration, a he hoa postdoctoral mua ma Caltech.

Ma mua o ka hanana GW230529, ua ʻike ʻia kekahi mea hoʻohiwahiwa nui ʻē aʻe. I kēlā hanana, i hana ʻia ma ʻAukake 2019 a ʻike ʻia ʻo GW190814, kahi Ua ʻike ʻia kahi mea paʻa o 2.6 ka nui o ka lā ma ke ʻano o ka hui ʻana o ka honua, akā ʻaʻole maopopo ka poʻe ʻepekema inā he hōkū neutron a i ʻole ʻeleʻele.

Ma hope o ka hoʻomaha ʻana no ka mālama ʻana a me ka hoʻomaikaʻi ʻana, e hoʻomaka hou ka holo ʻike ʻehā o nā mea ʻike ma ʻApelila 10, 2024, a e hoʻomau ʻia a hiki i Pepeluali 2025.

Kākau ʻia e Whitney Clavin

Source: Kāula



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