Marginal IR running of gravity as a natural explanation for dark matter

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dc.contributor.author Kumar, Naman
dc.coverage.spatial United States of America
dc.date.accessioned 2025-09-18T15:35:31Z
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
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.
dc.description.statementofresponsibility by Naman Kumar
dc.language.iso en_US
dc.publisher Cornell University Library
dc.title Marginal IR running of gravity as a natural explanation for dark matter
dc.type Article
dc.relation.journal arXiv


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