Matches in SemOpenAlex for { <https://semopenalex.org/work/W1499060571> ?p ?o ?g. }
- W1499060571 abstract "The recent claim by BICEP2 of evidence for primordial gravitational waves has focused interest on the potential for early-Universe cosmology using gravitational waves. In addition to cosmic microwave background detectors, efforts are underway to carry out gravitational-wave astronomy with pulsar timing arrays, space-based detectors, and terrestrial detectors. These efforts will probe a wide range of times in the early Universe, during which backgrounds may have been produced through processes such as phase transitions or preheating. We derive a rule of thumb (not so strong as an upper limit) governing the maximum energy density of cosmological backgrounds. For most scenarios, we expect the energy density spectrum to peak at values of ${mathrm{ensuremath{Omega}}}_{mathrm{gw}}(f)ensuremath{lesssim}1{0}^{ensuremath{-}12ifmmodepmelsetextpmfi{}2}$. We discuss the applicability of this rule and the implications for gravitational-wave astronomy." @default.
- W1499060571 created "2016-06-24" @default.
- W1499060571 creator A5082733295 @default.
- W1499060571 creator A5088976307 @default.
- W1499060571 date "2014-11-24" @default.
- W1499060571 modified "2023-10-17" @default.
- W1499060571 title "Estimates of maximum energy density of cosmological gravitational-wave backgrounds" @default.
- W1499060571 cites W1978916504 @default.
- W1499060571 cites W1984394478 @default.
- W1499060571 cites W1988326085 @default.
- W1499060571 cites W1990044200 @default.
- W1499060571 cites W1993387326 @default.
- W1499060571 cites W1998067752 @default.
- W1499060571 cites W2011913580 @default.
- W1499060571 cites W2012291066 @default.
- W1499060571 cites W2014058866 @default.
- W1499060571 cites W2018722100 @default.
- W1499060571 cites W2018726641 @default.
- W1499060571 cites W2019864432 @default.
- W1499060571 cites W2053150427 @default.
- W1499060571 cites W2053667643 @default.
- W1499060571 cites W2057521928 @default.
- W1499060571 cites W2057998845 @default.
- W1499060571 cites W2060583654 @default.
- W1499060571 cites W2073427735 @default.
- W1499060571 cites W2081511847 @default.
- W1499060571 cites W2092922530 @default.
- W1499060571 cites W2097530387 @default.
- W1499060571 cites W2100222488 @default.
- W1499060571 cites W2101904540 @default.
- W1499060571 cites W2117249822 @default.
- W1499060571 cites W2134251287 @default.
- W1499060571 cites W2142768579 @default.
- W1499060571 cites W2142809887 @default.
- W1499060571 cites W2153686825 @default.
- W1499060571 cites W2155678178 @default.
- W1499060571 cites W2156691056 @default.
- W1499060571 cites W2157264974 @default.
- W1499060571 cites W2164075972 @default.
- W1499060571 cites W2599810080 @default.
- W1499060571 cites W3023144861 @default.
- W1499060571 cites W3038096834 @default.
- W1499060571 cites W3098788446 @default.
- W1499060571 cites W3100108344 @default.
- W1499060571 cites W3104495286 @default.
- W1499060571 cites W3106338724 @default.
- W1499060571 cites W4244439594 @default.
- W1499060571 doi "https://doi.org/10.1103/physrevd.90.107502" @default.
- W1499060571 hasPublicationYear "2014" @default.
- W1499060571 type Work @default.
- W1499060571 sameAs 1499060571 @default.
- W1499060571 citedByCount "33" @default.
- W1499060571 countsByYear W14990605712015 @default.
- W1499060571 countsByYear W14990605712016 @default.
- W1499060571 countsByYear W14990605712017 @default.
- W1499060571 countsByYear W14990605712018 @default.
- W1499060571 countsByYear W14990605712019 @default.
- W1499060571 countsByYear W14990605712020 @default.
- W1499060571 countsByYear W14990605712021 @default.
- W1499060571 countsByYear W14990605712022 @default.
- W1499060571 countsByYear W14990605712023 @default.
- W1499060571 crossrefType "journal-article" @default.
- W1499060571 hasAuthorship W1499060571A5082733295 @default.
- W1499060571 hasAuthorship W1499060571A5088976307 @default.
- W1499060571 hasBestOaLocation W14990605712 @default.
- W1499060571 hasConcept C107195408 @default.
- W1499060571 hasConcept C110363677 @default.
- W1499060571 hasConcept C121332964 @default.
- W1499060571 hasConcept C1276947 @default.
- W1499060571 hasConcept C190330329 @default.
- W1499060571 hasConcept C207297109 @default.
- W1499060571 hasConcept C26405456 @default.
- W1499060571 hasConcept C2779557605 @default.
- W1499060571 hasConcept C44870925 @default.
- W1499060571 hasConcept C59375849 @default.
- W1499060571 hasConcept C62520636 @default.
- W1499060571 hasConcept C84999194 @default.
- W1499060571 hasConcept C85725439 @default.
- W1499060571 hasConceptScore W1499060571C107195408 @default.
- W1499060571 hasConceptScore W1499060571C110363677 @default.
- W1499060571 hasConceptScore W1499060571C121332964 @default.
- W1499060571 hasConceptScore W1499060571C1276947 @default.
- W1499060571 hasConceptScore W1499060571C190330329 @default.
- W1499060571 hasConceptScore W1499060571C207297109 @default.
- W1499060571 hasConceptScore W1499060571C26405456 @default.
- W1499060571 hasConceptScore W1499060571C2779557605 @default.
- W1499060571 hasConceptScore W1499060571C44870925 @default.
- W1499060571 hasConceptScore W1499060571C59375849 @default.
- W1499060571 hasConceptScore W1499060571C62520636 @default.
- W1499060571 hasConceptScore W1499060571C84999194 @default.
- W1499060571 hasConceptScore W1499060571C85725439 @default.
- W1499060571 hasFunder F4320306076 @default.
- W1499060571 hasIssue "10" @default.
- W1499060571 hasLocation W14990605711 @default.
- W1499060571 hasLocation W14990605712 @default.
- W1499060571 hasLocation W14990605713 @default.
- W1499060571 hasLocation W14990605714 @default.
- W1499060571 hasOpenAccess W1499060571 @default.
- W1499060571 hasPrimaryLocation W14990605711 @default.
- W1499060571 hasRelatedWork W2000706340 @default.