Hydrodynamic Origin of the 4.8 keV Migdal Effect Signal

preprint OA: closed
Full text JSON View at publisher

Abstract

Abstract Recent detection of a 5.01-sigma Migdal effect signal (UCAS, January 2026) revealed a mysterious 4.8 keV particle. Here we demonstrate that this signal is not a standalone dark matter candidate, but a localized excitation of a universal viscous fermion condensate (psi-field). By integrating laboratory data with astrophysical observations from XRISM and Chandra (6.2-sigma resonance), we show that the 4.8 keV mass dictates the cosmic viscosity (eta = 1.2e-15 Pa-s). This framework provides a single-parameter solution to the Hubble (H0) and S8 tensions, identifying the 4.8 keV fermion as the fundamental constituent of the space-time medium.
Full text 8,451 characters · extracted from preprint-html · click to expand
Hydrodynamic Origin of the 4.8 keV Migdal Effect Signal | Research Square window.SnipcartSettings = { analytics: { enabled: false } }; (function() { var accessVector = localStorage.getItem('access_vector') || ''; window.dataLayer = window.dataLayer || []; if (accessVector) { window.dataLayer.push({ user: { profile: { profileInfo: { snid: accessVector } } } }); } })(); (function(w,d,s,l,i){w[l]=w[l]||[];w[l].push({'gtm.start':new Date().getTime(),event:'gtm.js'});var f=d.getElementsByTagName(s)[0],j=d.createElement(s),dl=l!='dataLayer'?'&l='+l:'';j.async=true;j.src='https://www.googletagmanager.com/gtm.js?id='+i+dl;f.parentNode.insertBefore(j,f);})(window,document,'script','dataLayer','GTM-K279D39R'); Browse Preprints In Review Journals COVID-19 Preprints AJE Video Bytes Research Tools Research Promotion AJE Professional Editing AJE Rubriq About Preprint Platform In Review Editorial Policies Our Team Advisory Board Help Center Sign In Submit a Preprint Cite Share Download PDF Article Hydrodynamic Origin of the 4.8 keV Migdal Effect Signal Alexander Shlyapik This is a preprint; it has not been peer reviewed by a journal. https://doi.org/ 10.21203/rs.3.rs-8950310/v1 This work is licensed under a CC BY 4.0 License Status: Posted Version 1 posted You are reading this latest preprint version Abstract Recent detection of a 5.01-sigma Migdal effect signal (UCAS, January 2026) revealed a mysterious 4.8 keV particle. Here we demonstrate that this signal is not a standalone dark matter candidate, but a localized excitation of a universal viscous fermion condensate (psi-field). By integrating laboratory data with astrophysical observations from XRISM and Chandra (6.2-sigma resonance), we show that the 4.8 keV mass dictates the cosmic viscosity (eta = 1.2e-15 Pa-s). This framework provides a single-parameter solution to the Hubble (H0) and S8 tensions, identifying the 4.8 keV fermion as the fundamental constituent of the space-time medium. Physical sciences/Physics/Fluid dynamics Physical sciences/Physics/Astronomy and astrophysics/Dark energy and dark matter Full Text Additional Declarations There is NO Competing Interest. Cite Share Download PDF Status: Posted Version 1 posted You are reading this latest preprint version Research Square lets you share your work early, gain feedback from the community, and start making changes to your manuscript prior to peer review in a journal. As a division of Research Square Company, we’re committed to making research communication faster, fairer, and more useful. We do this by developing innovative software and high quality services for the global research community. Our growing team is made up of researchers and industry professionals working together to solve the most critical problems facing scientific publishing. Also discoverable on Platform About Our Team In Review Editorial Policies Advisory Board Help Center Resources Author Services Accessibility API Access RSS feed Manage Cookie Preferences © Research Square 2026 | ISSN 2693-5015 (online) Privacy Policy Terms of Service Do Not Sell My Personal Information {"props":{"pageProps":{"initialData":{"identity":"rs-8950310","acceptedTermsAndConditions":true,"allowDirectSubmit":true,"archivedVersions":[],"articleType":"Article","associatedPublications":[],"authors":[{"id":598423828,"identity":"cceb680e-5652-4ac5-883b-8e23da4bf761","order_by":0,"name":"Alexander Shlyapik","email":"data:image/png;base64,iVBORw0KGgoAAAANSUhEUgAAAZAAAAAyAQMAAABI0h/eAAAABlBMVEX///8AAABVwtN+AAAACXBIWXMAAA7EAAAOxAGVKw4bAAAA+ElEQVRIiWNgGAWjYBACAyjJIwGiE37YAEnGxgPEa3nYkwbS0kCEFiAAaWF8wHYYzMGrxZy999mDDwXbZCTbzxg+SOA5b7e2/TDQlhqbaFxaLHuOmxvOMLjNI82TY2yQYHE7eduZRKCWY2m5DbgcdiONTZoHqEWOIS1NIoHndrLZAaAWxobDuLXcfwbVwv8MqIXtXLLZ+YcEtNxgg2iRlkg+BtRywM7sBiFbzqSxg/0iOePxYYPEnuQEsxtAWxLw+eX4MbYHH/7ctpc4n9j48McPO3uz8+kPH3yoscGpBQjYUHiJYJUJuJVjarHHr3gUjIJRMApGIgAAcLphcXMQ3AEAAAAASUVORK5CYII=","orcid":"https://orcid.org/0009-0003-7726-109X","institution":"Independent Researcher","correspondingAuthor":true,"prefix":"","firstName":"Alexander","middleName":"","lastName":"Shlyapik","suffix":""}],"badges":[],"createdAt":"2026-02-23 19:50:31","currentVersionCode":1,"declarations":"","doi":"10.21203/rs.3.rs-8950310/v1","doiUrl":"https://doi.org/10.21203/rs.3.rs-8950310/v1","draftVersion":[],"editorialEvents":[],"editorialNote":"","failedWorkflow":false,"files":[{"id":103798795,"identity":"ffa77550-e9c8-42d5-9940-55ba879c03b8","added_by":"auto","created_at":"2026-03-03 05:14:32","extension":"pdf","order_by":1,"title":"","display":"","copyAsset":false,"role":"manuscript-pdf","size":221493,"visible":true,"origin":"","legend":"","description":"","filename":"HydrodynamicInterpretationofthe4.8keVMigdalEffectSignalasaViscousFermionCondensate.pdf","url":"https://assets-eu.researchsquare.com/files/rs-8950310/v1_covered_1ba79ccd-fbf9-4d5a-a4a8-d0b77da3cbb0.pdf"}],"financialInterests":"There is \u003cb\u003eNO\u003c/b\u003e Competing Interest.","formattedTitle":"Hydrodynamic Origin of the 4.8 keV Migdal Effect Signal","fulltext":[],"fulltextSource":"","fullText":"","funders":[],"hasAdminPriorityOnWorkflow":false,"hasManuscriptDocX":false,"hasOptedInToPreprint":true,"hasPassedJournalQc":"","hasAnyPriority":true,"hideJournal":true,"highlight":"","institution":"","isAcceptedByJournal":false,"isAuthorSuppliedPdf":true,"isDeskRejected":"","isHiddenFromSearch":false,"isInQc":false,"isInWorkflow":false,"isPdf":true,"isPdfUpToDate":true,"isWithdrawnOrRetracted":false,"journal":{"display":true,"email":"[email protected]","identity":"researchsquare","isNatureJournal":false,"hasQc":true,"allowDirectSubmit":true,"externalIdentity":"","sideBox":"","snPcode":"","submissionUrl":"/submission","title":"Research Square","twitterHandle":"researchsquare","acdcEnabled":true,"dfaEnabled":false,"editorialSystem":"","reportingPortfolio":"","inReviewEnabled":false,"inReviewRevisionsEnabled":true},"keywords":"","lastPublishedDoi":"10.21203/rs.3.rs-8950310/v1","lastPublishedDoiUrl":"https://doi.org/10.21203/rs.3.rs-8950310/v1","license":{"name":"CC BY 4.0","url":"https://creativecommons.org/licenses/by/4.0/"},"manuscriptAbstract":"Recent detection of a 5.01-sigma Migdal effect signal (UCAS, January 2026) revealed a mysterious 4.8 keV particle. Here we demonstrate that this signal is not a standalone dark matter candidate, but a localized excitation of a universal viscous fermion condensate (psi-field). By integrating laboratory data with astrophysical observations from XRISM and Chandra (6.2-sigma resonance), we show that the 4.8 keV mass dictates the cosmic viscosity (eta = 1.2e-15 Pa-s). This framework provides a single-parameter solution to the Hubble (H0) and S8 tensions, identifying the 4.8 keV fermion as the fundamental constituent of the space-time medium.","manuscriptTitle":"Hydrodynamic Origin of the 4.8 keV Migdal Effect Signal","msid":"","msnumber":"","nonDraftVersions":[{"code":1,"date":"2026-03-03 05:14:25","doi":"10.21203/rs.3.rs-8950310/v1","editorialEvents":[],"status":"published","journal":{"display":true,"email":"[email protected]","identity":"nature-physics","isNatureJournal":true,"hasQc":false,"allowDirectSubmit":false,"externalIdentity":"nphys","sideBox":"Learn more about [Nature Physics](http://www.nature.com/nphys/)","snPcode":"","submissionUrl":"","title":"Nature Physics","twitterHandle":"","acdcEnabled":true,"dfaEnabled":true,"editorialSystem":"ejp","reportingPortfolio":"Nature Research","inReviewEnabled":true,"inReviewRevisionsEnabled":false}}],"origin":"","ownerIdentity":"240ed309-0fb1-40ab-aec1-0c0ce09df843","owner":[],"postedDate":"March 3rd, 2026","published":true,"recentEditorialEvents":[],"rejectedJournal":[],"revision":"","amendment":"","status":"posted","subjectAreas":[{"id":63685077,"name":"Physical sciences/Physics/Fluid dynamics"},{"id":63685078,"name":"Physical sciences/Physics/Astronomy and astrophysics/Dark energy and dark matter"}],"tags":[],"updatedAt":"2026-03-03T12:30:12+00:00","versionOfRecord":[],"versionCreatedAt":"2026-03-03 05:14:25","video":"","vorDoi":"","vorDoiUrl":"","workflowStages":[]},"version":"v1","identity":"rs-8950310","journalConfig":"researchsquare"},"__N_SSP":true},"page":"/article/[identity]/[[...version]]","query":{"redirect":"/article/rs-8950310","identity":"rs-8950310","version":["v1"]},"buildId":"XKTyCvWXoU3ODBz1xrDgd","isFallback":false,"isExperimentalCompile":false,"dynamicIds":[84888],"gssp":true,"scriptLoader":[]}

Text is read by the "Ask this paper" AI Q&A widget below. Extraction quality varies by source — PMC NXML preserves structure cleanly, OA-HTML may include some navigation residue, and OA-PDF can have broken hyphenation. The publisher copy (via DOI) is the canonical version.

My notes (saved in your browser only)

Ask this paper AI returns verbatim quotes from the full text · source: preprint-html

Answers must be backed by verbatim quotes from this paper's full text. Hallucinated quotes are dropped automatically; if no verbatim passage answers the question, we say so. How this works

Citation neighborhood (no data yet)

We don't have any in-corpus citations linked to this paper yet. This is a recent paper (2026) — citers typically take a year or two to land, and the OpenAlex reference graph may still be filling in.

Source provenance

europepmc
last seen: 2026-05-20T01:45:00.602351+00:00