FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2950674963> ?p ?o ?g. }

• W2950674963 abstract "We have found the Quasi Normal Mode (QNM) frequencies of a class of static spherically symmetric spacetimes having a {it {smeared}} matter distribution, parameterized by $Theta$ - an inherent length scale. Here our main focus is on the QNMs for the odd parity perturbation in this background geometry. The results presented here for diffused mass distribution reveal significant changes in the QNM spectrum. This could be relevant for future generation (cosmological) observations, specifically to distinguish the signals of GW from a non-singular source in contrast to a singular geometry. We also provide numerical estimates for the $Theta$-corrected QNM spectrum applicable to typical globular cluster like spherical galaxies having a Gaussian spread in their mass distribution. We find that the $Theta$-correction to the GW signal due to smeared distribution is accessible to present day observational precision." @default.
• W2950674963 created "2019-06-27" @default.
• W2950674963 creator A5016709357 @default.
• W2950674963 creator A5040697764 @default.
• W2950674963 creator A5079634771 @default.
• W2950674963 date "2019-01-29" @default.
• W2950674963 modified "2023-09-24" @default.
• W2950674963 title "Quasinormal mode spectra for odd parity perturbations in spacetimes with smeared matter sources" @default.
• W2950674963 cites W1629749464 @default.
• W2950674963 cites W1968369949 @default.
• W2950674963 cites W1968833481 @default.
• W2950674963 cites W1973368884 @default.
• W2950674963 cites W1988899904 @default.
• W2950674963 cites W1989170879 @default.
• W2950674963 cites W1995217152 @default.
• W2950674963 cites W1997367763 @default.
• W2950674963 cites W1997874012 @default.
• W2950674963 cites W2013485448 @default.
• W2950674963 cites W2015757619 @default.
• W2950674963 cites W2029788031 @default.
• W2950674963 cites W2034527135 @default.
• W2950674963 cites W2050092976 @default.
• W2950674963 cites W2059049095 @default.
• W2950674963 cites W2059236649 @default.
• W2950674963 cites W2080705137 @default.
• W2950674963 cites W2082450121 @default.
• W2950674963 cites W2094338703 @default.
• W2950674963 cites W2104873160 @default.
• W2950674963 cites W2107259515 @default.
• W2950674963 cites W2121040900 @default.
• W2950674963 cites W2134783381 @default.
• W2950674963 cites W2144095749 @default.
• W2950674963 cites W2147829712 @default.
• W2950674963 cites W2166436681 @default.
• W2950674963 cites W2231773349 @default.
• W2950674963 cites W2252795400 @default.
• W2950674963 cites W2283318580 @default.
• W2950674963 cites W2296807820 @default.
• W2950674963 cites W2437571239 @default.
• W2950674963 cites W2621266390 @default.
• W2950674963 cites W2765081049 @default.
• W2950674963 cites W2778463638 @default.
• W2950674963 cites W2803139282 @default.
• W2950674963 cites W3004237104 @default.
• W2950674963 cites W3103204141 @default.
• W2950674963 doi "https://doi.org/10.1103/physrevd.99.024039" @default.
• W2950674963 hasPublicationYear "2019" @default.
• W2950674963 type Work @default.
• W2950674963 sameAs 2950674963 @default.
• W2950674963 citedByCount "2" @default.
• W2950674963 countsByYear W29506749632019 @default.
• W2950674963 crossrefType "journal-article" @default.
• W2950674963 hasAuthorship W2950674963A5016709357 @default.
• W2950674963 hasAuthorship W2950674963A5040697764 @default.
• W2950674963 hasAuthorship W2950674963A5079634771 @default.
• W2950674963 hasBestOaLocation W29506749631 @default.
• W2950674963 hasConcept C121332964 @default.
• W2950674963 hasConcept C124017977 @default.
• W2950674963 hasConcept C134222618 @default.
• W2950674963 hasConcept C163716315 @default.
• W2950674963 hasConcept C177918212 @default.
• W2950674963 hasConcept C190330329 @default.
• W2950674963 hasConcept C2777151079 @default.
• W2950674963 hasConcept C44870925 @default.
• W2950674963 hasConcept C4839761 @default.
• W2950674963 hasConcept C62520636 @default.
• W2950674963 hasConcept C74650414 @default.
• W2950674963 hasConcept C98444146 @default.
• W2950674963 hasConceptScore W2950674963C121332964 @default.
• W2950674963 hasConceptScore W2950674963C124017977 @default.
• W2950674963 hasConceptScore W2950674963C134222618 @default.
• W2950674963 hasConceptScore W2950674963C163716315 @default.
• W2950674963 hasConceptScore W2950674963C177918212 @default.
• W2950674963 hasConceptScore W2950674963C190330329 @default.
• W2950674963 hasConceptScore W2950674963C2777151079 @default.
• W2950674963 hasConceptScore W2950674963C44870925 @default.
• W2950674963 hasConceptScore W2950674963C4839761 @default.
• W2950674963 hasConceptScore W2950674963C62520636 @default.
• W2950674963 hasConceptScore W2950674963C74650414 @default.
• W2950674963 hasConceptScore W2950674963C98444146 @default.
• W2950674963 hasFunder F4320334771 @default.
• W2950674963 hasLocation W29506749631 @default.
• W2950674963 hasLocation W29506749632 @default.
• W2950674963 hasOpenAccess W2950674963 @default.
• W2950674963 hasPrimaryLocation W29506749631 @default.
• W2950674963 hasRelatedWork W1999364903 @default.
• W2950674963 hasRelatedWork W2025490324 @default.
• W2950674963 hasRelatedWork W2036897909 @default.
• W2950674963 hasRelatedWork W2607760299 @default.
• W2950674963 hasRelatedWork W2765124653 @default.
• W2950674963 hasRelatedWork W2765402880 @default.
• W2950674963 hasRelatedWork W2794432100 @default.
• W2950674963 hasRelatedWork W2885196600 @default.
• W2950674963 hasRelatedWork W2889307498 @default.
• W2950674963 hasRelatedWork W2915049909 @default.
• W2950674963 hasRelatedWork W2951226707 @default.
• W2950674963 hasRelatedWork W3016963506 @default.
• W2950674963 hasRelatedWork W3021885511 @default.
• W2950674963 hasRelatedWork W3080801237 @default.
• W2950674963 hasRelatedWork W3099154800 @default.

• next