Matches in SemOpenAlex for { <https://semopenalex.org/work/W2789042424> ?p ?o ?g. }
- W2789042424 endingPage "10" @default.
- W2789042424 startingPage "10" @default.
- W2789042424 abstract "The cold dark matter (CDM) paradigm successfully explains the cosmic structure over an enormous span of redshifts. However, it fails when probing the innermost regions of dark matter halos and the properties of the Milky Way’s dwarf galaxy satellites. Moreover, the lack of experimental detection of Weakly Interacting Massive Particle (WIMP) favors alternative candidates such as light axionic dark matter that naturally arise in string theory. Cosmological N-body simulations have shown that axionic dark matter forms a solitonic core of size of ≃150 pc in the innermost region of the galactic halos. The oscillating scalar field associated to the axionic dark matter halo produces an oscillating gravitational potential that induces a time dilation of the pulse arrival time of ≃400 ns/(m B /10 − 22 eV) for pulsar within such a solitonic core. Over the whole galaxy, the averaged predicted signal may be detectable with current and forthcoming pulsar timing array telescopes." @default.
- W2789042424 created "2018-03-06" @default.
- W2789042424 creator A5001342440 @default.
- W2789042424 creator A5017935883 @default.
- W2789042424 creator A5017999817 @default.
- W2789042424 creator A5025113934 @default.
- W2789042424 creator A5053635230 @default.
- W2789042424 creator A5074751129 @default.
- W2789042424 date "2018-01-16" @default.
- W2789042424 modified "2023-10-01" @default.
- W2789042424 title "Ultra Light Axionic Dark Matter: Galactic Halos and Implications for Observations with Pulsar Timing Arrays" @default.
- W2789042424 cites W1481345939 @default.
- W2789042424 cites W1500878904 @default.
- W2789042424 cites W1972633475 @default.
- W2789042424 cites W1984363547 @default.
- W2789042424 cites W1994627742 @default.
- W2789042424 cites W1997474154 @default.
- W2789042424 cites W2007746935 @default.
- W2789042424 cites W2009463540 @default.
- W2789042424 cites W2020177615 @default.
- W2789042424 cites W2022463172 @default.
- W2789042424 cites W2030979937 @default.
- W2789042424 cites W2033509750 @default.
- W2789042424 cites W2057899718 @default.
- W2789042424 cites W2062136406 @default.
- W2789042424 cites W2086100864 @default.
- W2789042424 cites W2102639000 @default.
- W2789042424 cites W2103678464 @default.
- W2789042424 cites W2110352019 @default.
- W2789042424 cites W2136355021 @default.
- W2789042424 cites W2397630455 @default.
- W2789042424 cites W2508641778 @default.
- W2789042424 cites W2594838509 @default.
- W2789042424 cites W2612259467 @default.
- W2789042424 cites W2612757325 @default.
- W2789042424 cites W2773395652 @default.
- W2789042424 cites W3005079263 @default.
- W2789042424 cites W3098136306 @default.
- W2789042424 cites W3099384065 @default.
- W2789042424 cites W3101735260 @default.
- W2789042424 cites W3102136416 @default.
- W2789042424 cites W3103675194 @default.
- W2789042424 cites W3126146816 @default.
- W2789042424 cites W67474965 @default.
- W2789042424 doi "https://doi.org/10.3390/galaxies6010010" @default.
- W2789042424 hasPublicationYear "2018" @default.
- W2789042424 type Work @default.
- W2789042424 sameAs 2789042424 @default.
- W2789042424 citedByCount "15" @default.
- W2789042424 countsByYear W27890424242018 @default.
- W2789042424 countsByYear W27890424242019 @default.
- W2789042424 countsByYear W27890424242020 @default.
- W2789042424 countsByYear W27890424242021 @default.
- W2789042424 countsByYear W27890424242022 @default.
- W2789042424 countsByYear W27890424242023 @default.
- W2789042424 crossrefType "journal-article" @default.
- W2789042424 hasAuthorship W2789042424A5001342440 @default.
- W2789042424 hasAuthorship W2789042424A5017935883 @default.
- W2789042424 hasAuthorship W2789042424A5017999817 @default.
- W2789042424 hasAuthorship W2789042424A5025113934 @default.
- W2789042424 hasAuthorship W2789042424A5053635230 @default.
- W2789042424 hasAuthorship W2789042424A5074751129 @default.
- W2789042424 hasBestOaLocation W27890424241 @default.
- W2789042424 hasConcept C121332964 @default.
- W2789042424 hasConcept C126320844 @default.
- W2789042424 hasConcept C1276947 @default.
- W2789042424 hasConcept C159249277 @default.
- W2789042424 hasConcept C172790937 @default.
- W2789042424 hasConcept C184665706 @default.
- W2789042424 hasConcept C26405456 @default.
- W2789042424 hasConcept C44870925 @default.
- W2789042424 hasConcept C57853336 @default.
- W2789042424 hasConcept C66157390 @default.
- W2789042424 hasConcept C88148261 @default.
- W2789042424 hasConcept C98444146 @default.
- W2789042424 hasConceptScore W2789042424C121332964 @default.
- W2789042424 hasConceptScore W2789042424C126320844 @default.
- W2789042424 hasConceptScore W2789042424C1276947 @default.
- W2789042424 hasConceptScore W2789042424C159249277 @default.
- W2789042424 hasConceptScore W2789042424C172790937 @default.
- W2789042424 hasConceptScore W2789042424C184665706 @default.
- W2789042424 hasConceptScore W2789042424C26405456 @default.
- W2789042424 hasConceptScore W2789042424C44870925 @default.
- W2789042424 hasConceptScore W2789042424C57853336 @default.
- W2789042424 hasConceptScore W2789042424C66157390 @default.
- W2789042424 hasConceptScore W2789042424C88148261 @default.
- W2789042424 hasConceptScore W2789042424C98444146 @default.
- W2789042424 hasIssue "1" @default.
- W2789042424 hasLocation W27890424241 @default.
- W2789042424 hasLocation W27890424242 @default.
- W2789042424 hasLocation W27890424243 @default.
- W2789042424 hasOpenAccess W2789042424 @default.
- W2789042424 hasPrimaryLocation W27890424241 @default.
- W2789042424 hasRelatedWork W1543597839 @default.
- W2789042424 hasRelatedWork W1972633475 @default.
- W2789042424 hasRelatedWork W1998523782 @default.
- W2789042424 hasRelatedWork W2019569420 @default.
- W2789042424 hasRelatedWork W2042163123 @default.