<?xml version="1.0" encoding="utf-8" standalone="yes"?><rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Posts | Luca Visinelli</title><link>https://lucavisinelli.com/post/</link><atom:link href="https://lucavisinelli.com/post/index.xml" rel="self" type="application/rss+xml"/><description>Posts</description><generator>Source Themes Academic (https://sourcethemes.com/academic/)</generator><language>en-us</language><copyright>© 2026 Luca Visinelli</copyright><lastBuildDate>Mon, 04 Aug 2025 10:11:33 +0000</lastBuildDate><image><url>https://lucavisinelli.com/media/pic1.jpg</url><title>Posts</title><link>https://lucavisinelli.com/post/</link></image><item><title>Neutrino masses from dark matter interactions?</title><link>https://lucavisinelli.com/post/neutrino-masses-from-dark-matter-interactions/</link><pubDate>Mon, 04 Aug 2025 10:11:33 +0000</pubDate><guid>https://lucavisinelli.com/post/neutrino-masses-from-dark-matter-interactions/</guid><description>&lt;p>Many articles have recently discussed the role of dark matter interactions as the origin of neutrino masses. This hypothesis can be practically tested in view of data from baseline and solar neutrino experiments, such as
&lt;a href="http://kamland.stanford.edu/" target="_blank" rel="noopener">KamLAND&lt;/a>. With
&lt;a href="https://inspirehep.net/authors/1790638" target="_blank" rel="noopener">Hong-Yi Zhang&lt;/a> and
&lt;a href="https://inspirehep.net/authors/1657730" target="_blank" rel="noopener">Andrew Cheek&lt;/a>, two postdocs at the
&lt;a href="https://tdli.sjtu.edu.cn/en/" target="_blank" rel="noopener">Tsung-Dao Lee Institute (TDLI)&lt;/a>, we have proceeded in this direction and carefully assessed the hypothesis. We found that current neutrino data strongly disfavors this scenario, especially when accounting for both temporal and spatial modulations of the dark matter field. Our work, recently published in
&lt;a href="https://journals.aps.org/prl/abstract/10.1103/wyns-m4y5" target="_blank" rel="noopener">Physical Review Letters&lt;/a>, sets new bounds on this class of models and helps sharpen the search for the true origin of neutrino mass.&lt;/p>
&lt;p>The preprint has recently received attention from Phys.org, which has covered the article in a popular science blog which is available at &lt;a href="https://phys.org/news/2025-07-neutrino-masses-interactions-dark.html">https://phys.org/news/2025-07-neutrino-masses-interactions-dark.html&lt;/a>. See also the press released by TDLI here: &lt;a href="https://mp.weixin.qq.com/s/nCmDFHN5hIirzIvGPKIwNg">https://mp.weixin.qq.com/s/nCmDFHN5hIirzIvGPKIwNg&lt;/a>.&lt;/p></description></item><item><title>Novel constraints on fifth forces and ultralight dark sector with asteroidal data</title><link>https://lucavisinelli.com/post/novel-constraints-on-fifth-forces-and-ultralight-dark-sector-with-asteroidal-data/</link><pubDate>Mon, 20 Mar 2023 08:09:15 +0000</pubDate><guid>https://lucavisinelli.com/post/novel-constraints-on-fifth-forces-and-ultralight-dark-sector-with-asteroidal-data/</guid><description>&lt;p>In
&lt;a href="https://arxiv.org/abs/2107.04038" target="_blank" rel="noopener">2107.04038&lt;/a>, my collaborators and myself have explored a novel idea: can high-quality asteroid data be used to constrain light bosons mediating a fifth force? This concept has been vastly covered by the lead author, Yu-Dai Tsai, in a Youtube interview available
&lt;a href="https://www.youtube.com/watch?v=xDX9XwLHBuM" target="_blank" rel="noopener">HERE&lt;/a>.&lt;/p>
&lt;p>The preprint has been now published in JCAP (2023), with the updated version appearing on the arXiv preprint service. In the meantime, we are working on extending the collaboration to include asteroid data analysis experts and refine the search in future publications.&lt;/p></description></item><item><title>Cambridge press release: have we detected dark energy?</title><link>https://lucavisinelli.com/post/cambridge-press-release-have-we-detected-dark-energy/</link><pubDate>Wed, 15 Sep 2021 16:26:46 +0000</pubDate><guid>https://lucavisinelli.com/post/cambridge-press-release-have-we-detected-dark-energy/</guid><description>&lt;p>My recently paper with
&lt;a href="https://www.sunnyvagnozzi.com/blog/welcome" target="_blank" rel="noopener">Sunny Vagnozzi&lt;/a>,
&lt;a href="https://phbrax.wixsite.com/brax" target="_blank" rel="noopener">Philippe Brax&lt;/a>,
&lt;a href="https://www.maths.cam.ac.uk/person/ad107" target="_blank" rel="noopener">Anne-Christine Davis&lt;/a>, and
&lt;a href="http://www.jeremysakstein.com" target="_blank" rel="noopener">Jeremy Sakstein &lt;/a>on the bold idea that a model of dark energy could be responsible for the
&lt;a href="https://cerncourier.com/a/researchers-grapple-with-xenon1t-excess/" target="_blank" rel="noopener">excess&lt;/a> reported by the
&lt;a href="http://www.xenon1t.org" target="_blank" rel="noopener">XENON-1T collaboration&lt;/a> is now published on
&lt;a href="https://journals.aps.org/prd/abstract/10.1103/PhysRevD.104.063023" target="_blank" rel="noopener">Physical Review D&lt;/a>. The arXiv preprint is available
&lt;a href="https://arxiv.org/abs/2103.15834" target="_blank" rel="noopener">at this link&lt;/a>.&lt;/p>
&lt;p>Our work has been covered by a press release of the University of Cambridge (home of Dr. Vagnozzi and Prof. Davis), which is found
&lt;a href="https://www.cam.ac.uk/research/news/have-we-detected-dark-energy-cambridge-scientists-say-its-a-possibility?fbclid=IwAR1ghM91ysIm7EGa2vDOC7I2nSGL32f7ewB1PSJ_QGB91g6hIO8Z-1x2R3s" target="_blank" rel="noopener">at this link&lt;/a>.&lt;/p>
&lt;p>More on the work is in
&lt;a href="https://lucavisinelli.com/post/can-we-detect-dark-energy-in-the-lab/" target="_blank" rel="noopener">my previous entry here&lt;/a>.&lt;/p></description></item><item><title>Can we detect dark energy in the lab?</title><link>https://lucavisinelli.com/post/can-we-detect-dark-energy-in-the-lab/</link><pubDate>Sun, 25 Jul 2021 07:14:33 +0000</pubDate><guid>https://lucavisinelli.com/post/can-we-detect-dark-energy-in-the-lab/</guid><description>&lt;p>Last year (June 2020), there has been a lot of excitement and speculation around the
&lt;a href="https://cerncourier.com/a/researchers-grapple-with-xenon1t-excess/" target="_blank" rel="noopener">excess&lt;/a> reported by the
&lt;a href="http://www.xenon1t.org" target="_blank" rel="noopener">XENON-1T collaboration&lt;/a>, which could be attributed to new physics such as the
&lt;a href="https://en.wikipedia.org/wiki/Axion" target="_blank" rel="noopener">axion&lt;/a>. I recently worked on the bold idea that a specific model of dark energy could have caused such an excess. My work with
&lt;a href="https://www.sunnyvagnozzi.com/blog/welcome" target="_blank" rel="noopener">Sunny Vagnozzi&lt;/a>,
&lt;a href="https://phbrax.wixsite.com/brax" target="_blank" rel="noopener">Philippe Brax&lt;/a>,
&lt;a href="https://www.maths.cam.ac.uk/person/ad107" target="_blank" rel="noopener">Anne-Christine Davis&lt;/a>, and
&lt;a href="http://www.jeremysakstein.com" target="_blank" rel="noopener">Jeremy Sakstein&lt;/a> is available on ArXiv
&lt;a href="https://arxiv.org/pdf/2103.15834" target="_blank" rel="noopener">at this link&lt;/a>. More excitingly, the model would be in reach of future experiments such as
&lt;a href="https://science.purdue.edu/xenon1t/?tag=xenonnt" target="_blank" rel="noopener">XENON-nT&lt;/a> and
&lt;a href="https://pandax.sjtu.edu.cn" target="_blank" rel="noopener">PandaX&lt;/a>.&lt;/p>
&lt;p>The preprint has recently received attention from Space.com, which has covered the article in a popular science blog which is available at &lt;a href="https://www.space.com/dark-energy-experiments-on-earth">https://www.space.com/dark-energy-experiments-on-earth&lt;/a>&lt;/p>
&lt;p>The research article by the XENON-1T collaboration on the reported excess can be found
&lt;a href="https://arxiv.org/pdf/2006.09721" target="_blank" rel="noopener">here&lt;/a>.&lt;/p></description></item><item><title>Media coverage of "Constraints on Stupendously Large Black Holes"</title><link>https://lucavisinelli.com/post/media-coverage-of-constraints-on-stupendously-large-black-holes/</link><pubDate>Sun, 09 May 2021 10:38:49 +0000</pubDate><guid>https://lucavisinelli.com/post/media-coverage-of-constraints-on-stupendously-large-black-holes/</guid><description>&lt;p>My work with Bernard Carr (Emeritus, Queen Mary University of London) and Florian Kühnel (Münich) on black holes is ranked #128 in all time media coverage of the Monthly Notices of the Royal Astronomical Society outputs.&lt;/p>
&lt;p>The published version of the paper is available on 
&lt;a href="https://doi.org/10.1093/mnras/staa3651" target="_blank" rel="noopener">&lt;em>Monthly Notices of the Royal Astronomical Society&lt;/em> &lt;strong>501&lt;/strong> (2) 2029–2043 (2021)&lt;/a>.&lt;/p>
&lt;p>Preprint: 
&lt;a href="https://arxiv.org/abs/2008.08077?fbclid=IwAR0q14CdeLPnxvCE5XQUvCHegALucLS0xnc1CGC_tHLKizEcFTVIMrO4-es" target="_blank" rel="noopener">https://arxiv.org/abs/2008.08077&lt;/a>; Press release of Queen Mary University of London
&lt;a href="https://www.qmul.ac.uk/media/news/2021/se/scientists-find-black-holes-could-reach-stupendously-large-sizes.html?fbclid=IwAR0mW4bX77pT0CV9C4zLlhuVwidQJGOAXJi6CTt6QE0VWI0tCIYFbomEHpw" target="_blank" rel="noopener">here&lt;/a>.&lt;/p>
&lt;p>
&lt;a href="https://www.altmetric.com/details/88479476#score" target="_blank" rel="noopener">Link to Altmetric webpage&lt;/a>.&lt;/p></description></item><item><title>Scientists find black holes could reach "stupendously large" sizes</title><link>https://lucavisinelli.com/post/scientists-find-black-holes-could-reach-stupendously-large-sizes/</link><pubDate>Fri, 22 Jan 2021 11:36:06 +0000</pubDate><guid>https://lucavisinelli.com/post/scientists-find-black-holes-could-reach-stupendously-large-sizes/</guid><description>&lt;p>A recent press coverage by
&lt;a href="https://www.qmul.ac.uk" target="_blank" rel="noopener">Queen Mary University of London&lt;/a> has focused on my work on black holes &lt;a href="https://arxiv.org/abs/2008.08077">https://arxiv.org/abs/2008.08077&lt;/a>.&lt;/p>
&lt;p>In the press coverage
&lt;a href="https://www.qmul.ac.uk/media/news/2021/se/scientists-find-black-holes-could-reach-stupendously-large-sizes.html" target="_blank" rel="noopener">available here&lt;/a> my collaborator
&lt;a href="https://www.qmul.ac.uk/spa/people/emeritus-staff/profiles/bjcarr.html" target="_blank" rel="noopener">Bernard Carr&lt;/a> of Queen Mary discusses in depth the outcome of our study and future projects. The paper has been recently published on
&lt;a href="https://doi.org/10.1093/mnras/staa3651" target="_blank" rel="noopener">&lt;em>Monthly Notices of the Royal Astronomical Society&lt;/em> &lt;strong>501&lt;/strong> (2) 2029–2043 (2021)&lt;/a>.&lt;/p></description></item><item><title>Non-Gaussianity from SM Higgs modulating inflaton decay</title><link>https://lucavisinelli.com/post/non-gaussianity-from-sm-higgs-modulating-inflaton-decay/</link><pubDate>Tue, 01 Dec 2020 10:31:09 +0000</pubDate><guid>https://lucavisinelli.com/post/non-gaussianity-from-sm-higgs-modulating-inflaton-decay/</guid><description>&lt;p>In two recent preprints (
&lt;a href="https://arxiv.org/abs/2011.05377" target="_blank" rel="noopener">&lt;/a>
&lt;a href="https://arxiv.org/abs/2011.11649" target="_blank" rel="noopener">2011.11649&lt;/a>,
&lt;a href="https://arxiv.org/abs/2009.14218" target="_blank" rel="noopener">2009.14218&lt;/a>), together with Aliki Litsa, Katherine Freese, Evangelos Sfakianakis, &amp;amp; Patrick Stengel, we discuss non-Gaussianity arising in the reheating process when the Higgs field modulates inflaton decay. This process is expected to arise even within a minimal Standard Model + inflaton setup and can be readily tested with upcoming probes, as we discuss at length in the preprints. This important work has been covered in great detail in &lt;a href="https://www.sunnyvagnozzi.com/blog/top-arxiv-week-48-2020">https://www.sunnyvagnozzi.com/blog/top-arxiv-week-48-2020&lt;/a>&lt;/p></description></item><item><title>Axion miniclusters and neutron stars</title><link>https://lucavisinelli.com/post/axion-miniclusters-and-neutron-stars/</link><pubDate>Mon, 16 Nov 2020 07:59:30 +0000</pubDate><guid>https://lucavisinelli.com/post/axion-miniclusters-and-neutron-stars/</guid><description>&lt;p>In two recent preprints available here (
&lt;a href="https://arxiv.org/abs/2011.05377" target="_blank" rel="noopener">2011.05377&lt;/a>,
&lt;a href="https://arxiv.org/abs/2011.05378" target="_blank" rel="noopener">2011.05378&lt;/a>), I have shown together with my colleagues Bradley Kavanagh, Thomas Edwards, and Christoph Weniger, that an encounter between a neutron star and an axion &lt;em>minicluster&lt;/em> would lead to a transient radio signal in the sky, which is potentially detectable. It took us 15 months to deliver the required code, which is available at &lt;a href="https://github.com/bradkav/axion-miniclusters/">https://github.com/bradkav/axion-miniclusters/&lt;/a>. This immense work has been covered in great detail here:
&lt;a href="https://www.sunnyvagnozzi.com/blog/top-arxiv-week-46-2020" target="_blank" rel="noopener">https://www.sunnyvagnozzi.com/blog/top-arxiv-week-46&lt;/a>&lt;/p></description></item><item><title>Black Holes and WIMPs blog coverage</title><link>https://lucavisinelli.com/post/black-holes-and-wimps-blog-coverage/</link><pubDate>Mon, 09 Nov 2020 15:00:18 +0000</pubDate><guid>https://lucavisinelli.com/post/black-holes-and-wimps-blog-coverage/</guid><description>&lt;p>My work on the interplay of black holes and WIMPs with Bernard Carr and Florian Kuhnel, available here (
&lt;a href="https://arxiv.org/abs/2011.01930" target="_blank" rel="noopener">arXiv:2011.01930&lt;/a>), has been covered in depth as one of the best papers of last week here:
&lt;a href="https://www.sunnyvagnozzi.com/blog/top-arxiv-week-45-2020?fbclid=IwAR2aN0sHOgeYHTQPv83Q4IycLJvitokUkggyeVDbTkA1KVUBdG9yH8FFei0" target="_blank" rel="noopener">https://www.sunnyvagnozzi.com/blog/top-arxiv-week-45&lt;/a>&lt;/p></description></item><item><title>'Stupendously large' black holes could grow to truly monstrous sizes</title><link>https://lucavisinelli.com/post/stupendously-large-black-holes-could-grow-to-truly-monstrous-sizes/</link><pubDate>Sun, 27 Sep 2020 17:11:59 +0000</pubDate><guid>https://lucavisinelli.com/post/stupendously-large-black-holes-could-grow-to-truly-monstrous-sizes/</guid><description>&lt;p>Coverage of my work on Primordial Black Holes in &lt;a href="https://arxiv.org/abs/2008.08077">https://arxiv.org/abs/2008.08077&lt;/a> appeared last week on space.com website here:&lt;/p>
&lt;p>&lt;a href="https://www.space.com/black-holes-can-reach-stupendously-large-sizes.html">https://www.space.com/black-holes-can-reach-stupendously-large-sizes.html&lt;/a>&lt;/p></description></item><item><title>Black holes – Do they grow stupendously large?</title><link>https://lucavisinelli.com/post/black-holes-do-they-grow-stupendously-large/</link><pubDate>Mon, 07 Sep 2020 19:08:42 +0000</pubDate><guid>https://lucavisinelli.com/post/black-holes-do-they-grow-stupendously-large/</guid><description>&lt;p>Coverage on popular science blog: &lt;a href="https://astrobites.org/2020/09/05/stupendously-large-black-holes/">https://astrobites.org/2020/09/05/stupendously-large-black-holes/&lt;/a>&lt;/p>
&lt;p>From my work on Primordial Black Holes in &lt;a href="https://arxiv.org/abs/2008.08077">https://arxiv.org/abs/2008.08077&lt;/a>&lt;/p></description></item><item><title>Interview on XENON for Il Messaggero (in Italian)</title><link>https://lucavisinelli.com/post/interview-on-xenon-for-il-messaggero-in-italian/</link><pubDate>Fri, 19 Jun 2020 19:35:34 +0000</pubDate><guid>https://lucavisinelli.com/post/interview-on-xenon-for-il-messaggero-in-italian/</guid><description>&lt;p>Interview for Il Messaggero (Italian newspaper with national coverage) on the XENON excess discovery in June 2020!&lt;/p>
&lt;p>&lt;a href="https://www.ilmessaggero.it/scienza/gran_sasso_esperimento_visinelli_18_giugno_2020-5295285.html">https://www.ilmessaggero.it/scienza/gran_sasso_esperimento_visinelli_18_giugno_2020-5295285.html&lt;/a>&lt;/p></description></item><item><title>Interview on Dark Matter</title><link>https://lucavisinelli.com/post/interview-on-dark-matter/</link><pubDate>Mon, 20 Apr 2020 19:53:06 +0000</pubDate><guid>https://lucavisinelli.com/post/interview-on-dark-matter/</guid><description>&lt;p>I have been interviewed by Il Messaggero, an Italian newspaper of national coverage, on the purpose of science, the profession of a physicist, and more specifically on the mystery of the dark matter here:
&lt;a href="https://www.ilmessaggero.it/scienza/materia_oscura_il_fisico_italiano_luca_visinelli_il_mistero_si_cela_dietro_a_una_particella-5155991.html" target="_blank" rel="noopener">https://www.ilmessaggero.it/scienza&lt;/a>&lt;/p></description></item><item><title>Interview with LUCA VISINELLI at Oskar Klein Centre, Stockholm</title><link>https://lucavisinelli.com/post/interviewokc/</link><pubDate>Fri, 07 Sep 2018 19:04:01 +0000</pubDate><guid>https://lucavisinelli.com/post/interviewokc/</guid><description>&lt;p>The interview I gave for public outreach at Oskar Klein Centre is available at &lt;a href="https://ssl.fysik.su.se/okc/internal/blog/interview-with-luca-visinelli/">https://ssl.fysik.su.se/okc/internal/blog/interview-with-luca-visinelli/&lt;/a>&lt;/p></description></item></channel></rss>