{"title":"Lorentz violation with an invariant minimum speed as foundation of the uncertainty principle in Minkowski, dS and AdS spaces","authors":"Cláudio Nassif Cruz","doi":"arxiv-2409.04925","DOIUrl":null,"url":null,"abstract":"This research aims to provide the geometrical foundation of the uncertainty\nprinciple within a new causal structure of spacetime so-called Symmetrical\nSpecial Relativity (SSR), where there emerges a Lorentz violation due to the\npresence of an invariant minimum speed $V$ related to the vacuum energy. SSR\npredicts that a dS-scenario occurs only for a certain regime of speeds $v$,\nwhere $v<v_0=\\sqrt{cV}$, which represents the negative gravitational potentials\n($\\Phi<0$) connected to the cosmological parameter $\\Lambda>0$. For $v=v_0$,\nMinkowski (pseudo-Euclidian) space is recovered for representing the flat space\n($\\Lambda=0$), and for $v>v_0$ ($\\Phi>0$), Anti-de Sitter (AdS) scenario\nprevails ($\\Lambda<0$). The fact that the current universe is flat as its\naverage density of matter distribution ($\\rho_m$ given for a slightly negative\ncurvature $R$) coincides with its vacuum energy density ($\\rho_{\\Lambda}$ given\nfor a slightly positive curvature $\\Lambda$), i.e., the {\\it cosmic coincidence\nproblem}, is now addressed by SSR. SSR provides its energy-momentum tensor of\nperfect fluid, leading to the EOS of vacuum ($p=-\\rho_{\\Lambda}$). Einstein\nequation for vacuum given by such SSR approach allows us to obtain\n$\\rho_{\\Lambda}$ associated with a scalar curvature $\\Lambda$, whereas the\nsolution of Einstein equation only in the presence of a homogeneous\ndistribution of matter $\\rho_m$ for the whole universe presents a scalar\ncurvature $R$, in such a way that the presence of the background field\n$\\Lambda$ opposes the Riemannian curvature $R$, thus leading to a current\neffective curvature $R_{eff}=R+\\Lambda\\approx 0$ according to observations.","PeriodicalId":501041,"journal":{"name":"arXiv - PHYS - General Relativity and Quantum Cosmology","volume":"34 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-09-07","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv - PHYS - General Relativity and Quantum Cosmology","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2409.04925","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
Abstract
This research aims to provide the geometrical foundation of the uncertainty
principle within a new causal structure of spacetime so-called Symmetrical
Special Relativity (SSR), where there emerges a Lorentz violation due to the
presence of an invariant minimum speed $V$ related to the vacuum energy. SSR
predicts that a dS-scenario occurs only for a certain regime of speeds $v$,
where $v0$. For $v=v_0$,
Minkowski (pseudo-Euclidian) space is recovered for representing the flat space
($\Lambda=0$), and for $v>v_0$ ($\Phi>0$), Anti-de Sitter (AdS) scenario
prevails ($\Lambda<0$). The fact that the current universe is flat as its
average density of matter distribution ($\rho_m$ given for a slightly negative
curvature $R$) coincides with its vacuum energy density ($\rho_{\Lambda}$ given
for a slightly positive curvature $\Lambda$), i.e., the {\it cosmic coincidence
problem}, is now addressed by SSR. SSR provides its energy-momentum tensor of
perfect fluid, leading to the EOS of vacuum ($p=-\rho_{\Lambda}$). Einstein
equation for vacuum given by such SSR approach allows us to obtain
$\rho_{\Lambda}$ associated with a scalar curvature $\Lambda$, whereas the
solution of Einstein equation only in the presence of a homogeneous
distribution of matter $\rho_m$ for the whole universe presents a scalar
curvature $R$, in such a way that the presence of the background field
$\Lambda$ opposes the Riemannian curvature $R$, thus leading to a current
effective curvature $R_{eff}=R+\Lambda\approx 0$ according to observations.