<?xml version="1.0"?><rdf:RDF xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:edm="http://www.europeana.eu/schemas/edm/" xmlns:wgs84_pos="http://www.w3.org/2003/01/geo/wgs84_pos" xmlns:foaf="http://xmlns.com/foaf/0.1/" xmlns:rdaGr2="http://rdvocab.info/ElementsGr2" xmlns:oai="http://www.openarchives.org/OAI/2.0/" xmlns:owl="http://www.w3.org/2002/07/owl#" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:ore="http://www.openarchives.org/ore/terms/" xmlns:skos="http://www.w3.org/2004/02/skos/core#" xmlns:dcterms="http://purl.org/dc/terms/"><edm:WebResource rdf:about="http://www.dlib.si/stream/URN:NBN:SI:DOC-EJJW8DKM/17bf2f1d-0c33-440d-b71d-fbf44a7b8f4f/IMAGE"><dcterms:extent>124 KB</dcterms:extent></edm:WebResource><edm:WebResource rdf:about="http://www.dlib.si/stream/URN:NBN:SI:DOC-EJJW8DKM/776badc1-dc85-47ce-825a-c1c8266e420a/PDF"><dcterms:extent>1651 KB</dcterms:extent></edm:WebResource><edm:WebResource rdf:about="http://www.dlib.si/stream/URN:NBN:SI:DOC-EJJW8DKM/ab82c3c6-44ea-4251-b09d-fb68570777b2/TEXT"><dcterms:extent>37 KB</dcterms:extent></edm:WebResource><edm:ProvidedCHO rdf:about="URN:NBN:SI:DOC-EJJW8DKM"><dcterms:issued>2025</dcterms:issued><dc:creator>Pestotnik Stres, Luna</dc:creator><dc:format xml:lang="sl">1 spletni vir (1 datoteka PDF (22 str.))</dc:format><dc:identifier>COBISSID:247658243</dc:identifier><dc:identifier>ISBN:978-961-93233-6-6</dc:identifier><dc:identifier>URN:URN:NBN:SI:doc-EJJW8DKM</dc:identifier><dc:language>en</dc:language><dc:publisher xml:lang="sl">Stres inženiring</dc:publisher><dc:source xml:lang="sl">knjige</dc:source><dc:title xml:lang="sl">Determining the elongation of a rod in different gravitational fields of a black hole|</dc:title><dc:description xml:lang="sl">This work explores the elongation of a steel rod in the gravitational fields of black holes of different masses, comparing constant and variable field approximations. Using stress–strain relationships and Newton’s law of gravitation, elongation and maximum rod length before fracture were calculated. Results show that gravitational gradients significantly increase elongation near black holes, with smaller black holes producing stronger stretching effects. The analysis demonstrates how extreme gravitational fields influence material deformation, linking astrophysical conditions to mechanical limits</dc:description><edm:type>TEXT</edm:type><dc:type xml:lang="sl">knjige</dc:type><dc:type xml:lang="en">books</dc:type><dc:type rdf:resource="http://www.wikidata.org/entity/Q571" /></edm:ProvidedCHO><ore:Aggregation rdf:about="http://www.dlib.si/?URN=URN:NBN:SI:DOC-EJJW8DKM"><edm:aggregatedCHO rdf:resource="URN:NBN:SI:DOC-EJJW8DKM" /><edm:isShownBy rdf:resource="http://www.dlib.si/stream/URN:NBN:SI:DOC-EJJW8DKM/776badc1-dc85-47ce-825a-c1c8266e420a/PDF" /><edm:rights rdf:resource="http://rightsstatements.org/vocab/InC/1.0/" /><edm:provider>Slovenian National E-content Aggregator</edm:provider><edm:intermediateProvider xml:lang="en">National and University Library of Slovenia</edm:intermediateProvider><edm:dataProvider xml:lang="sl">Narodna in študijska knjižnica</edm:dataProvider><edm:object rdf:resource="http://www.dlib.si/streamdb/URN:NBN:SI:DOC-EJJW8DKM/maxi/edm" /><edm:isShownAt rdf:resource="http://www.dlib.si/details/URN:NBN:SI:DOC-EJJW8DKM" /></ore:Aggregation></rdf:RDF>