dc.contributor.author |
Kumar, Naman |
|
dc.coverage.spatial |
United States of America |
|
dc.date.accessioned |
2025-09-18T15:35:31Z |
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dc.date.available |
2025-09-18T15:35:31Z |
|
dc.date.issued |
2025-09 |
|
dc.identifier.citation |
Kumar, Naman, "Marginal IR running of gravity as a natural explanation for dark matter", arXiv, Cornell University Library, DOI: arXiv:2509.05246, Sep. 2025. |
|
dc.identifier.issn |
2331-8422 |
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dc.identifier.uri |
https://doi.org/10.48550/arXiv.2509.05246 |
|
dc.identifier.uri |
https://repository.iitgn.ac.in/handle/123456789/12145 |
|
dc.description.abstract |
We propose that the infrared (IR) running of Newton's coupling provides a simple and universal explanation for large--distance modifications of gravity relevant to dark matter phenomenology. Within the effective field theory (EFT) framework, we model G(k) as a scale--dependent coupling governed by an anomalous dimension \eta. We show that the marginal case \eta = 1 is singled out by renormalization group (RG) and dimensional arguments, leading to a logarithmic potential and a 1/r force law at large distances, while smoothly recovering Newtonian gravity at short scales. The logarithmic correction is universal and regulator independent, indicating that the 1/r force arises as the robust IR imprint of quantum--field--theoretic scaling. This provides a principled alternative to particle dark matter, suggesting that galactic rotation curves and related anomalies may be understood as manifestations of the IR running of Newton's constant. |
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dc.description.statementofresponsibility |
by Naman Kumar |
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dc.language.iso |
en_US |
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dc.publisher |
Cornell University Library |
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dc.title |
Marginal IR running of gravity as a natural explanation for dark matter |
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dc.type |
Article |
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dc.relation.journal |
arXiv |
|