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		<doi>10.1007/s10509-014-2121-6</doi>
		<issn>0004-640X</issn>
		<label>lattes: 9527086189389353 2 MoraesMira:2014:CoBrTe</label>
		<citationkey>MoraesMira:2014:CoBrTe</citationkey>
		<title>Constraining the brane tension in Randall-Sundrum cosmology through gravitational waves from binary neutron stars</title>
		<year>2014</year>
		<month>September 2014</month>
		<typeofwork>journal article</typeofwork>
		<secondarytype>PRE PI</secondarytype>
		<numberoffiles>1</numberoffiles>
		<size>317 KiB</size>
		<author>Moraes, Pedro Henrique Ribeiro da Silva,</author>
		<author>Miranda, Oswaldo Duarte,</author>
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		<group>AST-CEA-SPG-INPE-MCTI-GOV-BR</group>
		<group>CEA-CEA-INPE-MCTI-GOV-BR</group>
		<affiliation>Instituto Nacional de Pesquisas Espaciais (INPE)</affiliation>
		<affiliation>Instituto Nacional de Pesquisas Espaciais (INPE)</affiliation>
		<e-mailaddress>marcelo.pazos@inpe.br</e-mailaddress>
		<journal>Astrophysics and Space Science</journal>
		<volume>354</volume>
		<number>2</number>
		<pages>645-649</pages>
		<secondarymark>B1_GEOCIÊNCIAS B3_MATEMÁTICA_/_PROBABILIDADE_E B3_ASTRONOMIA_/_FÍSICA</secondarymark>
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		<keywords>Cosmologia, Objetos Compactos, Estrelas de Nêutrons, Ondas Gravitacionais, Dimensões Extras.</keywords>
		<abstract>When describing our world as a brane embedded in a higher dimensional hypersurface (or bulk) we are led to consider the existence of some new parameters related to the extra dimension or to the brane itself, as the brane tension density parameter &#937;&#955;. We show that gravitational waves emitted by binary neutron stars can constrain the values that &#937;&#955; might assume. Our approach is applied to the perspectives of Einstein Telescope gravitational wave detector and results in &#937;&#955; &#8804; 0.037, which is in agreement with other estimates obtained from different methods in the literature.</abstract>
		<area>CEA</area>
		<language>en</language>
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		<notes>Setores de Atividade: Pesquisa e desenvolvimento científico.</notes>
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