The inequalities of Bell, Clauser-Horne-Shimony-Holt (CHSH) and others are shown to be inconsistent with the Fundamental (Universal) Model of probability theory when combined with physics laws of the Malus-type. This combination permits the modeling of all results of quantum theory related to CHSH-Aspect-type experiments, while respecting Einstein’s separation principle
{"title":"Malus-Law Models for Aspect-Type Experiments","authors":"K. Hess","doi":"10.4236/jmp.2023.148064","DOIUrl":"https://doi.org/10.4236/jmp.2023.148064","url":null,"abstract":"The inequalities of Bell, Clauser-Horne-Shimony-Holt (CHSH) and others are shown to be inconsistent with the Fundamental (Universal) Model of probability theory when combined with physics laws of the Malus-type. This combination permits the modeling of all results of quantum theory related to CHSH-Aspect-type experiments, while respecting Einstein’s separation principle","PeriodicalId":70853,"journal":{"name":"现代物理(英文)","volume":null,"pages":null},"PeriodicalIF":0.0,"publicationDate":"2023-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"70394606","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"An Alternative View: Satisfaction of the Four-Variable Bell Inequality Using Quantum Correlations","authors":"L. Sica","doi":"10.4236/jmp.2023.148069","DOIUrl":"https://doi.org/10.4236/jmp.2023.148069","url":null,"abstract":"","PeriodicalId":70853,"journal":{"name":"现代物理(英文)","volume":null,"pages":null},"PeriodicalIF":0.0,"publicationDate":"2023-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"70394793","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2023-01-01DOI: 10.4236/jmp.2023.1410074
Keith G. Lyon
{"title":"Magnetic Charge Theory Part 4: Fermion Angular Momentum","authors":"Keith G. Lyon","doi":"10.4236/jmp.2023.1410074","DOIUrl":"https://doi.org/10.4236/jmp.2023.1410074","url":null,"abstract":"","PeriodicalId":70853,"journal":{"name":"现代物理(英文)","volume":null,"pages":null},"PeriodicalIF":0.0,"publicationDate":"2023-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"70391499","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"A Model of Accelerated Expansion of the Universe Based on the Idea about a Hypothetical 4-Dimensial Substance with an Inverse Population of Energy Levels","authors":"E. P. Orlov","doi":"10.4236/jmp.2023.141001","DOIUrl":"https://doi.org/10.4236/jmp.2023.141001","url":null,"abstract":"","PeriodicalId":70853,"journal":{"name":"现代物理(英文)","volume":null,"pages":null},"PeriodicalIF":0.0,"publicationDate":"2023-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"70391835","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"A Review of Recent Trends in Quantum Thermodynamics and a System’s Behavioural Analysis of the Universe Originating as a Quantum Energy System","authors":"S. Palmer","doi":"10.4236/jmp.2023.141004","DOIUrl":"https://doi.org/10.4236/jmp.2023.141004","url":null,"abstract":"","PeriodicalId":70853,"journal":{"name":"现代物理(英文)","volume":null,"pages":null},"PeriodicalIF":0.0,"publicationDate":"2023-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"70391858","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"A Model of Modified Newtonian Gravity Alternative to MOND, Consistent with the Properties of Spiral Galaxies and Compatible with Extragalactic Dark Matter","authors":"M. Rybicki","doi":"10.4236/jmp.2023.141005","DOIUrl":"https://doi.org/10.4236/jmp.2023.141005","url":null,"abstract":"","PeriodicalId":70853,"journal":{"name":"现代物理(英文)","volume":null,"pages":null},"PeriodicalIF":0.0,"publicationDate":"2023-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"70391902","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"A Physical Explanation for the Formation of Auroras","authors":"W. Qian","doi":"10.4236/jmp.2023.143018","DOIUrl":"https://doi.org/10.4236/jmp.2023.143018","url":null,"abstract":"","PeriodicalId":70853,"journal":{"name":"现代物理(英文)","volume":null,"pages":null},"PeriodicalIF":0.0,"publicationDate":"2023-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"70393379","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
In 1998, two groups of astronomers set out to determine the deceleration of the universe by measuring the recession speeds of type la supernovae (SN1a), came to an unexpected conclusion: its expansion rate has been speeding up. To justify this acceleration, they suggested that the universe does have a mysterious dark energy and they have proposed a positive cosmological constant consistent with the image of an inflationary universe. To explain the observed dimming of high-redshift SN1a they have bet on their distance revised upwards. We consider that an accelerated expansion leads right to a «dark energy catastrophe» and we suppose rather that the universe knows a slowdown expansion under the positive pressure of a dark energy, otherwise called a variable cosmological constant. The dark luminosity of the latter would be that of a «tired light» which has lost energy with distance. As for the low brilliance of SN1a, it is explained by two physical processes: The first relates to their intrinsic brightness – supposedly do not vary over time – which would depend on the chemical conditions which change with the temporal evolution; The second would concern their apparent luminosity. Besides the serious arguments already known, we strongly propose that their luminosity continually fades by interactions with cosmic magnetic fields, like the earthly PVLAS experiment which loses much more laser photons than expected by crossing a magnetic field. It goes in the sense of a «tired light» which has lost energy with distance and, therefore, a decelerated expansion of the universe.
{"title":"Cosmological Inconstant, Supernovae 1a and Decelerating Expansion","authors":"Russell Bagdoo","doi":"10.4236/jmp.2023.145040","DOIUrl":"https://doi.org/10.4236/jmp.2023.145040","url":null,"abstract":"In 1998, two groups of astronomers set out to determine the deceleration of the universe by measuring the recession speeds of type la supernovae (SN1a), came to an unexpected conclusion: its expansion rate has been speeding up. To justify this acceleration, they suggested that the universe does have a mysterious dark energy and they have proposed a positive cosmological constant consistent with the image of an inflationary universe. To explain the observed dimming of high-redshift SN1a they have bet on their distance revised upwards. We consider that an accelerated expansion leads right to a «dark energy catastrophe» and we suppose rather that the universe knows a slowdown expansion under the positive pressure of a dark energy, otherwise called a variable cosmological constant. The dark luminosity of the latter would be that of a «tired light» which has lost energy with distance. As for the low brilliance of SN1a, it is explained by two physical processes: The first relates to their intrinsic brightness – supposedly do not vary over time – which would depend on the chemical conditions which change with the temporal evolution; The second would concern their apparent luminosity. Besides the serious arguments already known, we strongly propose that their luminosity continually fades by interactions with cosmic magnetic fields, like the earthly PVLAS experiment which loses much more laser photons than expected by crossing a magnetic field. It goes in the sense of a «tired light» which has lost energy with distance and, therefore, a decelerated expansion of the universe.","PeriodicalId":70853,"journal":{"name":"现代物理(英文)","volume":null,"pages":null},"PeriodicalIF":0.0,"publicationDate":"2023-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"70393851","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Spherically Symmetric Problem of General Relativity for an Elastic Solid Sphere","authors":"V. Vasiliev, L. Fedorov","doi":"10.4236/jmp.2023.146047","DOIUrl":"https://doi.org/10.4236/jmp.2023.146047","url":null,"abstract":"","PeriodicalId":70853,"journal":{"name":"现代物理(英文)","volume":null,"pages":null},"PeriodicalIF":0.0,"publicationDate":"2023-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"70394115","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Quantum-Relativistic Properties of the Space-Time Bubbles and Their Evolution in a Multi-Bubble Universe","authors":"Massimo Auci","doi":"10.4236/jmp.2023.147058","DOIUrl":"https://doi.org/10.4236/jmp.2023.147058","url":null,"abstract":"","PeriodicalId":70853,"journal":{"name":"现代物理(英文)","volume":null,"pages":null},"PeriodicalIF":0.0,"publicationDate":"2023-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"70394163","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
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