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Bounding the Cosmological Constant using Galactic Rotation Curves from the SPARC Dataset

Bounding the Cosmological Constant using Galactic Rotation Curves from the SPARC Dataset

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_3097949940

Bounding the Cosmological Constant using Galactic Rotation Curves from the SPARC Dataset

About this item

Full title

Bounding the Cosmological Constant using Galactic Rotation Curves from the SPARC Dataset

Publisher

Ithaca: Cornell University Library, arXiv.org

Journal title

arXiv.org, 2024-08

Language

English

Formats

Publication information

Publisher

Ithaca: Cornell University Library, arXiv.org

More information

Scope and Contents

Contents

Dark energy (and its simplest model, the Cosmological Constant or \(\Lambda\)) acts as a repulsive force that opposes gravitational attraction. Assuming galaxies maintain a steady state over extended periods, the estimated upper limit on \(\Lambda\) studies its pushback to the attractive gravitational force of dark matter. From the SPARC dataset, w...

Alternative Titles

Full title

Bounding the Cosmological Constant using Galactic Rotation Curves from the SPARC Dataset

Authors, Artists and Contributors

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_journals_3097949940

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_3097949940

Other Identifiers

E-ISSN

2331-8422

DOI

10.48550/arxiv.2405.16650

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