Search for anti-quark nuggets via their interaction with the LHC beam

Fuente: arXiv

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Bibliographic Details
Main Authors:	Zioutas, K., Zhitnitsky, A., Zamantzas, C., Semertzidis, Y. K., Ruimi, O. M., Ozbozduman, K., Maroudas, M., Kryemadhi, A., Karuza, M., Horns, D., Gougas, A., Cetin, S., Cantatore, G., Budker, D.
Format:	Preprint
Published:	2024
Subjects:	High Energy Physics - Experiment Instrumentation and Methods for Astrophysics High Energy Physics - Phenomenology
Online Access:	Acceder al recurso
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author	Zioutas, K. Zhitnitsky, A. Zamantzas, C. Semertzidis, Y. K. Ruimi, O. M. Ozbozduman, K. Maroudas, M. Kryemadhi, A. Karuza, M. Horns, D. Gougas, A. Cetin, S. Cantatore, G. Budker, D.
author_facet	Zioutas, K. Zhitnitsky, A. Zamantzas, C. Semertzidis, Y. K. Ruimi, O. M. Ozbozduman, K. Maroudas, M. Kryemadhi, A. Karuza, M. Horns, D. Gougas, A. Cetin, S. Cantatore, G. Budker, D.
contents	Anti-quark nuggets (AQNs) have been suggested to solve the dark matter (DM) and the missing antimatter problem in the universe and have been proposed as an explanation of various observations. Their size is in the μm range and their density is about equal to the nuclear density with an expected flux of about $0.4 / km^2 / year$. For the typical velocity of DM constituents ($\sim$250 km/s), the solar system bodies act as highly performing gravitational lenses. Here we assume that DM streams or clusters are impinging, e.g., on the Earth, as it was worked out for DM axions and Weakly Interacting Massive Particles (WIMPs). Interestingly, in the LHC beam, unforeseen beam losses are triggered by so-called Unidentified Falling Objects (UFOs), which are believed to be constituted of dust particles with a size in the μm range and a density of several orders of magnitude lower than AQNs. Prezeau suggested that streaming DM constituents incident on the Earth should result in jet-like structures ("hairs") exiting the Earth, or a kind of caustics. Such ideas open novel directions in the search for DM. This work suggests a new analysis of the UFO results at the Large Hadron Collider (LHC), assuming that they are eventually, at least partly, due to AQNs. Firstly, a reanalysis of the existing data from the 4000 beam monitors since the beginning of the LHC is proposed, arguing that dust and AQNs should behave differently. The feasibility of this idea has been discussed with CERN accelerator people and potential collaborators.
format	Preprint
id	arxiv_https___arxiv_org_abs_2403_05608
institution	arXiv
publishDate	2024
record_format	arxiv
spellingShingle	Search for anti-quark nuggets via their interaction with the LHC beam Zioutas, K. Zhitnitsky, A. Zamantzas, C. Semertzidis, Y. K. Ruimi, O. M. Ozbozduman, K. Maroudas, M. Kryemadhi, A. Karuza, M. Horns, D. Gougas, A. Cetin, S. Cantatore, G. Budker, D. High Energy Physics - Experiment Instrumentation and Methods for Astrophysics High Energy Physics - Phenomenology Anti-quark nuggets (AQNs) have been suggested to solve the dark matter (DM) and the missing antimatter problem in the universe and have been proposed as an explanation of various observations. Their size is in the μm range and their density is about equal to the nuclear density with an expected flux of about $0.4 / km^2 / year$. For the typical velocity of DM constituents ($\sim$250 km/s), the solar system bodies act as highly performing gravitational lenses. Here we assume that DM streams or clusters are impinging, e.g., on the Earth, as it was worked out for DM axions and Weakly Interacting Massive Particles (WIMPs). Interestingly, in the LHC beam, unforeseen beam losses are triggered by so-called Unidentified Falling Objects (UFOs), which are believed to be constituted of dust particles with a size in the μm range and a density of several orders of magnitude lower than AQNs. Prezeau suggested that streaming DM constituents incident on the Earth should result in jet-like structures ("hairs") exiting the Earth, or a kind of caustics. Such ideas open novel directions in the search for DM. This work suggests a new analysis of the UFO results at the Large Hadron Collider (LHC), assuming that they are eventually, at least partly, due to AQNs. Firstly, a reanalysis of the existing data from the 4000 beam monitors since the beginning of the LHC is proposed, arguing that dust and AQNs should behave differently. The feasibility of this idea has been discussed with CERN accelerator people and potential collaborators.
title	Search for anti-quark nuggets via their interaction with the LHC beam
topic	High Energy Physics - Experiment Instrumentation and Methods for Astrophysics High Energy Physics - Phenomenology
url	https://arxiv.org/abs/2403.05608