FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3104417541> ?p ?o ?g. }

• W3104417541 endingPage "31" @default.
• W3104417541 startingPage "24" @default.
• W3104417541 abstract "We study the non-linear gravitational collapse of dark matter into halos through numerical N-body simulations of Lemaitre-Tolman-Bondi void models. We extend the halo mass function formalism to these models in a consistent way. This extension not only compares well with the simulated data at all times and radii, but it also gives interesting clues about the impact of the background shear on the growth of perturbations. Our results give hints about the possibility of constraining the background shear via cluster number counts, which could then give rise to strong constraints on general inhomogeneous models, of any scale." @default.
• W3104417541 created "2020-11-23" @default.
• W3104417541 creator A5004460370 @default.
• W3104417541 creator A5011635269 @default.
• W3104417541 creator A5057299715 @default.
• W3104417541 creator A5076755949 @default.
• W3104417541 date "2012-11-01" @default.
• W3104417541 modified "2023-10-18" @default.
• W3104417541 title "Halo abundances and shear in void models" @default.
• W3104417541 cites W1595531539 @default.
• W3104417541 cites W1895140248 @default.
• W3104417541 cites W1969438240 @default.
• W3104417541 cites W1973368884 @default.
• W3104417541 cites W2003182532 @default.
• W3104417541 cites W2004800095 @default.
• W3104417541 cites W2013354694 @default.
• W3104417541 cites W2021759576 @default.
• W3104417541 cites W2029234737 @default.
• W3104417541 cites W2029763831 @default.
• W3104417541 cites W2032412243 @default.
• W3104417541 cites W2033267528 @default.
• W3104417541 cites W2042956136 @default.
• W3104417541 cites W2059384534 @default.
• W3104417541 cites W2069176876 @default.
• W3104417541 cites W2072544006 @default.
• W3104417541 cites W2092548700 @default.
• W3104417541 cites W2101568531 @default.
• W3104417541 cites W2110795238 @default.
• W3104417541 cites W2118568439 @default.
• W3104417541 cites W2130954332 @default.
• W3104417541 cites W2134712793 @default.
• W3104417541 cites W2135329062 @default.
• W3104417541 cites W2162787896 @default.
• W3104417541 cites W2167450417 @default.
• W3104417541 cites W2170752525 @default.
• W3104417541 cites W3037700368 @default.
• W3104417541 cites W3098221464 @default.
• W3104417541 cites W3100260643 @default.
• W3104417541 cites W3100685670 @default.
• W3104417541 cites W3102644315 @default.
• W3104417541 cites W3102887027 @default.
• W3104417541 cites W3125925571 @default.
• W3104417541 doi "https://doi.org/10.1016/j.dark.2012.08.001" @default.
• W3104417541 hasPublicationYear "2012" @default.
• W3104417541 type Work @default.
• W3104417541 sameAs 3104417541 @default.
• W3104417541 citedByCount "12" @default.
• W3104417541 countsByYear W31044175412012 @default.
• W3104417541 countsByYear W31044175412013 @default.
• W3104417541 countsByYear W31044175412014 @default.
• W3104417541 countsByYear W31044175412015 @default.
• W3104417541 countsByYear W31044175412016 @default.
• W3104417541 countsByYear W31044175412018 @default.
• W3104417541 countsByYear W31044175412020 @default.
• W3104417541 countsByYear W31044175412022 @default.
• W3104417541 crossrefType "journal-article" @default.
• W3104417541 hasAuthorship W3104417541A5004460370 @default.
• W3104417541 hasAuthorship W3104417541A5011635269 @default.
• W3104417541 hasAuthorship W3104417541A5057299715 @default.
• W3104417541 hasAuthorship W3104417541A5076755949 @default.
• W3104417541 hasBestOaLocation W31044175411 @default.
• W3104417541 hasConcept C121332964 @default.
• W3104417541 hasConcept C121864883 @default.
• W3104417541 hasConcept C124017977 @default.
• W3104417541 hasConcept C127313418 @default.
• W3104417541 hasConcept C142362112 @default.
• W3104417541 hasConcept C153349607 @default.
• W3104417541 hasConcept C159249277 @default.
• W3104417541 hasConcept C159985019 @default.
• W3104417541 hasConcept C184665706 @default.
• W3104417541 hasConcept C192562407 @default.
• W3104417541 hasConcept C2778106948 @default.
• W3104417541 hasConcept C2779772531 @default.
• W3104417541 hasConcept C44870925 @default.
• W3104417541 hasConcept C558565934 @default.
• W3104417541 hasConcept C57879066 @default.
• W3104417541 hasConcept C5900021 @default.
• W3104417541 hasConcept C73301696 @default.
• W3104417541 hasConcept C74650414 @default.
• W3104417541 hasConcept C88148261 @default.
• W3104417541 hasConcept C96035792 @default.
• W3104417541 hasConcept C98444146 @default.
• W3104417541 hasConceptScore W3104417541C121332964 @default.
• W3104417541 hasConceptScore W3104417541C121864883 @default.
• W3104417541 hasConceptScore W3104417541C124017977 @default.
• W3104417541 hasConceptScore W3104417541C127313418 @default.
• W3104417541 hasConceptScore W3104417541C142362112 @default.
• W3104417541 hasConceptScore W3104417541C153349607 @default.
• W3104417541 hasConceptScore W3104417541C159249277 @default.
• W3104417541 hasConceptScore W3104417541C159985019 @default.
• W3104417541 hasConceptScore W3104417541C184665706 @default.
• W3104417541 hasConceptScore W3104417541C192562407 @default.
• W3104417541 hasConceptScore W3104417541C2778106948 @default.
• W3104417541 hasConceptScore W3104417541C2779772531 @default.
• W3104417541 hasConceptScore W3104417541C44870925 @default.
• W3104417541 hasConceptScore W3104417541C558565934 @default.
• W3104417541 hasConceptScore W3104417541C57879066 @default.
• W3104417541 hasConceptScore W3104417541C5900021 @default.

• next