{"title":"作为闵科夫斯基空间、dS 空间和 AdS 空间不确定性原理基础的具有最小速度不变性的洛伦兹违反现象","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":"{\"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}","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}
Lorentz violation with an invariant minimum speed as foundation of the uncertainty principle in Minkowski, dS and AdS spaces
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.