{"id":109,"date":"2021-08-12T13:44:36","date_gmt":"2021-08-12T13:44:36","guid":{"rendered":"https:\/\/revistabrasileiradefisica.com\/rbf\/?p=109"},"modified":"2021-11-24T09:59:13","modified_gmt":"2021-11-24T12:59:13","slug":"e202108010101-introducao-aos-buracos-negros","status":"publish","type":"post","link":"https:\/\/revistabrasileiradefisica.com\/rbf\/2021\/08\/12\/e202108010101-introducao-aos-buracos-negros\/","title":{"rendered":"Introdu\u00e7\u00e3o aos buracos negros"},"content":{"rendered":"\n<h4 class=\"wp-block-heading\"><em>A black holes introduction<\/em><\/h4>\n\n\n\n<p class=\"has-small-font-size\"><strong>DOI<\/strong>: <em><a href=\"https:\/\/doi.org\/10.5281\/zenodo.5188081\">10.5281\/zenodo.5188081<\/a><\/em><\/p>\n\n\n\n<p class=\"has-small-font-size\"><strong>Tiago Cardoso Floriano<\/strong> <br><em>Universidade Federal de Santa Maria<\/em><br><em><a rel=\"noreferrer noopener\" href=\"https:\/\/orcid.org\/0000-0003-3560-1028\" target=\"_blank\">ORCID<\/a> | <a href=\"http:\/\/lattes.cnpq.br\/5835989184892454\" target=\"_blank\" rel=\"noreferrer noopener\">Lattes<\/a> | <a href=\"mailto:tiago.floriano@acad.ufsm.br\">E-mail<\/a><\/em><\/p>\n\n\n\n<p class=\"has-small-font-size\"><strong>Resumo: <\/strong>O fim de algumas estrelas pode ser se tornar uma nebulosa ap\u00f3s uma explos\u00e3o catacl\u00edsmica, criando um ambiente prop\u00edcio para a forma\u00e7\u00e3o de novas estrelas e semeando os objetos pr\u00f3ximos com os elementos qu\u00edmicos que a constitu\u00eda, ou se tornar uma estrela de n\u00eautrons, dependendo do que sobrou da explos\u00e3o. Uma outra possibilidade, a depender do qu\u00e3o pesada est\u00e1 a estrela, que n\u00e3o tem mais for\u00e7as para vencer a gravidade, \u00e9 entrar em colapso gravitacional e tornar-se um buraco negro. O objetivo deste artigo \u00e9 fornecer uma vis\u00e3o geral que sirva de introdu\u00e7\u00e3o para o estudo de t\u00f3picos relacionados a estes objetos.<br><strong>Palavras-chave:<\/strong> buracos negros; relatividade geral; gravita\u00e7\u00e3o.<\/p>\n\n\n\n<p class=\"has-small-font-size\"><em><strong>Abstract: <\/strong>The end of some stars can be to become a nebula after a cataclysmic explosion, creating an environment conducive to the formation of new stars and seeding nearby objects with the chemical elements that made it up, or becoming a neutron star, depending on what left over from the explosion. Another possibility, depending on how heavy a star is that it no longer has the strength to overcome gravity, is to collapse gravitationally and become a black hole. The purpose of this article is to provide an overview that serves as an introduction to the study of topics related to these objects.<\/em><br><em><strong>Keywords: <\/strong>black holes; general relativity; gravitation.<\/em><\/p>\n\n\n\n<div class=\"wp-block-buttons is-layout-flex\">\n<div class=\"wp-block-button\"><a class=\"wp-block-button__link\" href=\"https:\/\/doi.org\/10.5281\/zenodo.5188081\" target=\"_blank\" rel=\"noreferrer noopener\">Baixar em PDF<\/a><\/div>\n<\/div>\n\n\n\n<p><\/p>\n","protected":false},"excerpt":{"rendered":"<p>A black holes introduction DOI: 10.5281\/zenodo.5188081 Tiago Cardoso Floriano Universidade Federal de Santa MariaORCID | Lattes | E-mail Resumo: O fim de algumas estrelas pode [&#8230;]<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"_mi_skip_tracking":false,"_monsterinsights_sitenote_active":false,"_monsterinsights_sitenote_note":"","_monsterinsights_sitenote_category":0},"categories":[24],"tags":[19,22,21,20,173],"_links":{"self":[{"href":"https:\/\/revistabrasileiradefisica.com\/rbf\/wp-json\/wp\/v2\/posts\/109"}],"collection":[{"href":"https:\/\/revistabrasileiradefisica.com\/rbf\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/revistabrasileiradefisica.com\/rbf\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/revistabrasileiradefisica.com\/rbf\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/revistabrasileiradefisica.com\/rbf\/wp-json\/wp\/v2\/comments?post=109"}],"version-history":[{"count":9,"href":"https:\/\/revistabrasileiradefisica.com\/rbf\/wp-json\/wp\/v2\/posts\/109\/revisions"}],"predecessor-version":[{"id":249,"href":"https:\/\/revistabrasileiradefisica.com\/rbf\/wp-json\/wp\/v2\/posts\/109\/revisions\/249"}],"wp:attachment":[{"href":"https:\/\/revistabrasileiradefisica.com\/rbf\/wp-json\/wp\/v2\/media?parent=109"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/revistabrasileiradefisica.com\/rbf\/wp-json\/wp\/v2\/categories?post=109"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/revistabrasileiradefisica.com\/rbf\/wp-json\/wp\/v2\/tags?post=109"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}