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  1. Time Remains.Sean Gryb & Karim P. Y. Thébault - 2016 - British Journal for the Philosophy of Science 67 (3):663-705.
    On one popular view, the general covariance of gravity implies that change is relational in a strong sense, such that all it is for a physical degree of freedom to change is for it to vary with regard to a second physical degree of freedom. At a quantum level, this view of change as relative variation leads to a fundamentally timeless formalism for quantum gravity. Here, we will show how one may avoid this acute ‘problem of time’. Under our view, (...)
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  2. On an Intrinsic Quantum Theoretical Structure Inside Einstein's Gravity Field Equations.Han Geurdes - manuscript
    As is well known, Einstein was dissatisfied with the foundation of quantum theory and sought to find a basis for it that would have satisfied his need for a causal explanation. In this paper this abandoned idea is investigated. It is found that it is mathematically not dead at all. More in particular: a quantum mechanical U(1) gauge invariant Dirac equation can be derived from Einstein's gravity field equations. We ask ourselves what it means for physics, the history of physics (...)
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  3. Field Equations, Quantum Mechanics and Geotropism.Han J. F. Geurdes - manuscript
    The biochemistry of geotropism in plants and gravisensing in e.g. cyanobacteria or paramacia is still not well understood today [1]. Perhaps there are more ways than one for organisms to sense gravity. The two best known relatively old explanations for gravity sensing are sensing through the redistribution of cellular starch statoliths and sensing through redistribution of auxin. The starch containing statoliths in a gravity field produce pressure on the endoplasmic reticulum of the cell. This enables the cell to sense direction. (...)
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  4. On an Intrinsic Quantum Theoretical Structure Inside Einstein's Gravity Field Equations.J. F. Geurdes - manuscript
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  5. On Curved Spacetime.Sydney Ernest Grimm - manuscript
    Albert Einstein’s theory of General Relativity was once the leading theory in theoretical physics. Unfortunately the theory describes macroscopic reality without a clear link with the the microcosm in respect to the properties of spacetime. However the theory of General Relativity has proved to predict macroscopic phenomena in a very accurate way. Nowadays most theoretical physicists use the conceptual framework of quantum theory. So it is not surprisingly that the question about the “true nature” of spacetime becomes very intrigue.
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  6. The Dark Energy as Effect on Gravitational Field.Joao Carlos Holland - manuscript
    We will make a new approach for an effect known as “Dark Energy” by an effect on gravitational field. In an accelerated rocket, the dimensions of space towards movement due to ‘Lorentz Contraction’ are on continuous reduction. Using the equivalence principle, we presume that in the gravitational field, the same thing would happen. In this implicates in ‘dark energy effect’. The calculi show that in a 7%-contraction for each billion years would explain our observation of galaxies in accelerated separation.
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  7. An Alternative to the Schwarzschild Solution of GTR.Andrew Thomas Holster - manuscript
    The Schwarzschild solution (Schwarzschild, 1915/16) to Einstein’s General Theory of Relativity (GTR) is accepted in theoretical physics as the unique solution to GTR for a central-mass system. In this paper I propose an alternative solution to GTR, and argue it is both logically consistent and empirically realistic as a theory of gravity. This solution is here called K-gravity. The introduction explains the basic concept. The central sections go through the technical detail, defining the basic solution for the geometric tensor, the (...)
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  8. Matters of Time Directionality in Classical and Quantum Physics.Jean-Christophe Lindner - manuscript
    This report offers a modern perspective on the question of time directionality as it arises in a classical and quantum mechanical context, based on key developments in the field of gravitational physics. Important clarifications are achieved regarding, in particular, the concepts of time reversal, negative energy and causality. From this analysis emerges an improved understanding of the general relativistic concept of stress-energy of matter as being a manifestation of local variations in the energy density of zero-point vacuum fluctuations. Based on (...)
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  9. 2. Programming Relativity as the Mathematics of Perspective in a Planck Unit Simulation Hypothesis.Malcolm Macleod - manuscript
    The Simulation Hypothesis proposes that all of reality is in fact an artificial simulation, analogous to a computer simulation. Outlined here is a method for programming relativistic mass, space and time at the Planck level as applicable for use in Planck Universe-as-a-Simulation Hypothesis. For the virtual universe the model uses a 4-axis hyper-sphere that expands in incremental steps (the simulation clock-rate). Virtual particles that oscillate between an electric wave-state and a mass point-state are mapped within this hyper-sphere, the oscillation driven (...)
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  10. 3. Planck Unit Quantum Gravity (Gravitons) for Simulation Hypothesis Modeling.Malcolm J. Macleod - manuscript
    Defined are gravitational formulas in terms of Planck units and units of $\hbar c$. Mass is not assigned as a constant property but is instead treated as a discrete event defined by units of Planck mass with gravity as an interaction between these units, the gravitational orbit as the sum of these mass-mass interactions and the gravitational coupling constant as a measure of the frequency of these interactions and not the magnitude of the gravitational force itself. Each particle that is (...)
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  11. From McTaggart to AdS_5 Geometry 2.Paul Merriam - manuscript
    The purpose of this note is to show how an 'AB-series' interpretation of time, given in a companion paper, leads, surprisingly, to AdS_5 geometry. This is not a theory of 2 time dimensions. Rather, it is a theory of 1 time dimension that has both A-series and B-series characteristics.
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  12. From McTaggart to AdS_5 Geometry V. 3.Paul Merriam - manuscript
    The purpose of this note is to show how an 'AB-series' interpretation of time leads, surprisingly, apparently, to AdS_5 geometry. This is not a theory of 2 time dimensions. Rather, it is a theory of 1 time dimension that has both A-series and B-series characteristics. To summarize the result, a spacetime in terms of (1) the earlier-to-later aspect of time, and (2) the (related) future-present-past aspect of time, and (3) 3-d space, it would seem, gives us the AdS_5 geometry.
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  13. McTaggart Saves Schrodinger's Cat?Paul Merriam - manuscript
    This paper proposes an interpretation of time that is an 'A-theory' in that it incorporates both McTaggart's A-series and his B-series. The A-series characteristics are supposed to be 'ontologically private' analogous to qualia in the Inverted Spectrum thought experiment and is given a definition. It is proposed one may define a 'unit of becoming' that coordinatizes the future/present/past spectrum as well as allowing one to calculate the rates of becoming. We give a picture of this interpretation and discuss how it (...)
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  14. McTaggart Saves Schrodinger's Cat?Paul Merriam - manuscript
    This paper proposes an interpretation of time that is an 'A-theory' in that it incorporates both McTaggart's A-series and his B-series. The A-series characteristics are supposed to be 'ontologically private' analogous to qualia in the Inverted Spectrum thought experiment and is given a definition. The main idea is that the experimenter and the cat do not share the same A-series characteristics. So there is no single time at which the cat gets ascribed different states. It is proposed one may define (...)
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  15. Schrodinger's Cat Meets McTaggart and the Problem of Other Minds.Paul Merriam - manuscript
    This paper proposes an interpretation of time that is an 'A-theory' in that it incorporates both McTaggart's A-series and his B-series. The A-series characteristics are supposed to be 'ontologically private' analogous to qualia in the problem of other minds and is given a definition. The main idea is that the experimenter and the cat do not share the same A-series characteristics, e.g the same 'now'. So there is no single time at which the cat gets ascribed different states. It is (...)
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  16. Anomalies de la relativité générale.Sfetcu Nicolae - manuscript
    Au fil du temps, la théorie de la relativité générale a accumulé plusieurs anomalies, indiquant la nécessité de meilleures théories sur la gravité ou d'autres approches. Les hypothèses ad hoc introduites en relativité générale pour expliquer les singularités gravitationnelles basées sur les conditions énergétiques ne sont pas très efficaces. Des hypothèses plus détaillées sur le contenu du sujet sont nécessaires . De nombreux scientifiques et philosophes sont parvenus à la conclusion que les singularités doivent être associées à l'atteinte des limites (...)
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  17. Observations cosmologiques pour la vérification de la relativité générale.Sfetcu Nicolae - manuscript
    Les scientifiques espèrent qu'à l'avenir ils pourront tester des trous noirs en observant les effets causés par un fort champ gravitationnel à proximité, comme la lentille gravitationnelle. Il existe déjà des observations sur les lentilles gravitationnelles faibles, dans lesquelles les rayons lumineux sont déviés en quelques secondes seulement, mais jamais directement pour un trou noir. Il existe plusieurs candidats à cet effet, en orbite autour du Sagittaire A*. Plusieurs conjectures ad hoc ont été introduites pour mieux expliquer les observations de (...)
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  18. Quantum Mechanics Foundations.Bakytzhan Oralbekov - manuscript
    Gravity remains the most elusive field. Its relationship with the electromagnetic field is poorly understood. Relativity and quantum mechanics describe the aforementioned fields, respectively. Bosons and fermions are often credited with responsibility for the interactions of force and matter. It is shown here that fermions factually determine the gravitational structure of the universe, while bosons are responsible for the three established and described forces. Underlying the relationships of the gravitational and electromagnetic fields is a symmetrical probability distribution of fermions and (...)
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  19. Ontologie de la relativité générale.Nicolae Sfetcu - manuscript
    Dans la vision classique, l'espace et le temps sont des conteneurs ; la matière est le contenu. La propriété distinctive de la matière est qu'elle transporte de l'énergie et des impulsions, préservée dans le temps, ce qui donne à ces impulsions un caractère ontologique fondamental. La relativité générale a généré diverses interprétations philosophiques anciennes. Ses adhérents ont mis en avant la « relativisation de l'inertie » et le concept de simultanéité, les kantiens et les néo-kantiens ont souligné l'approche de certaines (...)
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  20. Teste gravitaționale ale relativității generale.Nicolae Sfetcu - manuscript
    Perioada dintre 1960 și 1980 a fost perioada de maturitate a relativității generale: s-au dezvoltat noi metode de testare de mare precizie care au inclus teste noi, precum precesiunea giroscopică, întârzierea luminii și "efectul Nordtvedt" în mișcarea lunară, utilizând inclusiv observații astrofizice și sateliții artificiali. Există diferențe mari de predicții între relativitatea generală și fizica clasică, precum dilatarea timpului gravitațional, lentila gravitațională, deplasarea spre roșu gravitațională a luminii, etc. Și există multe teorii relativiste ale gravitației, bifurcate sau independente, dar teoria (...)
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  21. Heuristics of the General Relativity.Nicolae Sfetcu - manuscript
    The general theory of relativity was developed using as a nucleus a principle of symmetry: the principle of general covariance. Initially, Einstein saw the principle of general covariance as an extension of the principle of relativity in classical mechanics, and in SR. For Einstein, the principle of general covariance was a crucial postulate in the development of GR. The freedom of the GR diffeomorphism (the invariance of the form of the laws under transformations of the coordinates depending on the arbitrary (...)
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  22. Singularități gravitaționale.Nicolae Sfetcu - manuscript
    Singularitățile gravitaționale în relativitatea generală sunt locații în spațiu-timp unde câmpul gravitațional devine infinit. Curburile invariabile scalare ale spațiu-timpului includ o măsură a densității materiei. Unii fizicieni și filosofi consideră că, deoarece densitatea materiei tinde spre infinit în singularitate, legile spațiu-timpului nu mai sunt valabile acolo. O singularitățile gravitațională aproape unanim acceptată în astrofizică și cosmologie, ca cea mai timpurie stare a universului, este Big Bang. Nici în acest caz legile cunoscute ale fizicii nu mai sunt valabile. DOI: 10.13140/RG.2.2.27271.75681.
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  23. Epistemology of General Relativity.Nicolae Sfetcu - manuscript
    For Einstein, simplicity is the main criterion in the theoretical choice when the experiments and observations do not give sufficiently clear indications . Univocity in the theoretical representation of nature should not be confused with a denial of the underdetermination thesis. The principle of univocality played a central role in Einstein's formulation of general relativity. According to Einstein, a constructive theory offers a constructive model for phenomena of interest. A principle theory consists of a set of well-substantiated individual empirical generalizations. (...)
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  24. Ontology of Gravitational Singularities.Nicolae Sfetcu - manuscript
    General relativity allows singularities, and we need to understand the ontology of singularities if we want to understand the nature of space and time in the present universe. Although some physicists believe that singularities indicate a failure of general relativity, others believe that singularities open a new horizon in cosmology, with real physical phenomena that can help deepen our understanding of the world. From the definitions of singularities, most known are the possibility that some spacetimes contain incomplete paths (most accepted), (...)
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  25. Teste gravitaționale cosmologice.Nicolae Sfetcu - manuscript
    Modelele cosmologice actuale sunt construite pe baza relativității generale. Soluțiile ecuațiilor specifice, Friedmann-Lemaître-Robertson-Walker permit modelarea evoluției universului pornind de la Big Bang. O parte din parametrii universului au fost stabiliți prin observații. Pe baza acestora, și altor date observaționale, se pot testa modelele. Predicțiile includ abundența inițială de elemente chimice formate într-o perioadă de nucleosinteză în perioada Big Bang, structura ulterioară a universului, radiația cosmică de fond, etc. DOI: 10.13140/RG.2.2.22204.59525.
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  26. Introduction dans les théories de la relativité.Nicolae Sfetcu - manuscript
    Selon la relativité générale, la force gravitationnelle est une manifestation de la géométrie de l'espace-temps local. RG est une théorie métrique de la gravité. Il est basé sur les équations d'Einstein, qui décrivent la relation entre la géométrie d'une variété pseudo-riemannienne à quatre dimensions, représentant l'espace-temps et l'énergie-impulsion contenu dans cet espace-temps. La gravité correspond aux modifications des propriétés spatiales et temporelles, qui à leur tour modifient les chemins des objets. La courbure est causée par l'énergie-impulsion de la matière. Selon (...)
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  27. Singularités gravitationnelles.Nicolae Sfetcu - manuscript
    Les singularités gravitationnelles dans la relativité générale sont des emplacements dans l'espace-temps où le champ gravitationnel devient infini. Les courbes scalaires invariantes de l'espace-temps incluent une mesure de la densité de la matière. Certains physiciens et philosophes estiment que, du fait que la densité de la matière tend vers l'infini dans la singularité, les lois de l'espace-temps ne sont plus valables là-bas. Le Big Bang est une singularité gravitationnelle acceptée presque unanimement en astrophysique et en cosmologie, en tant que premier (...)
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  28. Evaluation of Post-Einsteinian Gravitational Theories Through Parameterized Post-Newtonian Formalism.Nicolae Sfetcu - manuscript
    Right after the elaboration and success of general relativity (GR), alternative theories for gravity began to appear. In order to verify and classify all these theories, specific tests have been developed, based on self-consistency and on completeness. In the field of experimental gravity, one of the important applications is formalism. For the evaluation of gravity models, several sets of tests have been proposed. Parameterized post-Newtonian formalism considers approximations of Einstein's gravity equations by the lowest order deviations from Newton's law for (...)
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  29. Ontologia relativității generale.Nicolae Sfetcu - manuscript
    Relativitatea generală a generat diverse interpretări filosofice timpurii. Adepții lui au evidențiat "relativizarea inerției" și conceptul de simultaneitate, kantienii și neo-kantienii au subliniat abordarea anumitor "forme intelectuale" sintetice (în special principiul covarianței generale, iar empiriștii logici au accentuat semnificația filozofică metodologică a teoriei. Reichenbach a abordat relativitatea generală prin prisma tezei "relativității geometriei", încercând o "axiomatizare constructivă" a teoriei relativității pe baza "problemelor elementare de fapt" (Elementaratbestande) cu privire la comportamentul observabil al razelor de lumină, a tijelor și a ceasurilor. (...)
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  30. Teste gravitaționale în câmp puternic.Nicolae Sfetcu - manuscript
    Când densitatea corpului devine suficient de mare, relativitatea generală prezice formarea unei găuri negre. Stelele neutronice de circa 1,4 mase solare și găurile negre sunt starea finală pentru evoluția stelelor masive. De obicei o gaură neagră într-o galaxie a jucat un rol important în formarea acesteia și a structurilor cosmice aferente. Astfel de corpuri oferă un mecanism eficient pentru emisia de radiații electromagnetice și formarea de microquasari. Accreția poate duce la jeturi relativiste. Relativitatea generală permite modelarea acestor fenomene, confirmate prin (...)
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  31. Anomalii ale relativității generale.Nicolae Sfetcu - manuscript
    În timp, teoria generală a relativității a acumulat mai multe anomalii și discrepanțe, indicând necesitatea unor teorii mai bune despre gravitație sau alte moduri de abordare. Ipotezele ad-hoc introduse în relativitatea generală pentru a explica singularitățile gravitaționale pe baza condițiilor energetice nu sunt foarte eficiente. Sunt necesare ipoteze mai detaliate asupra conținutului materiei. Mulți oameni de știință și filosofi au ajuns la concluzia că singularitățile trebuie să fie asociate cu atingerea limitelor valabilității fizice a relativității generale, fiind nevoie să se (...)
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  32. L'ontologie des singularités.Nicolae Sfetcu - manuscript
    La relativité générale permet les singularités et nous devons comprendre l'ontologie si nous voulons comprendre la nature de l'espace et du temps dans l'univers d'aujourd'hui. Bien que certains physiciens pensent que les singularités indiquent un échec de la relativité générale, d'autres pensent que les singularités ouvrent un nouvel horizon dans la cosmologie, avec de réels phénomènes physiques pouvant contribuer à un progrès profond dans notre compréhension du monde. DOI: 10.13140/RG.2.2.24491.18728 .
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  33. Teorii alternative la relativitatea generală – Formalismul PPN.Nicolae Sfetcu - manuscript
    Imediat după elaborarea și succesul relativității generale, au început să apară teorii alternative pentru gravitație. În dezvoltarea acestor teorii s-au încercat multe strategii (euristici pozitive) diferite, prin adăugarea de noi ipoteze la TGR, utilizarea unui spațiu-timp pentru care universul este static, ipoteze care elimină singularitățile gravitaționale, etc. Pentru evaluarea modelelor de gravitație, au fost propuse mai multe seturi de teste. Formalismul post-newtonian ia în considerare aproximări ale ecuațiilor de gravitație ale lui Einstein prin abaterile de ordinul cel mai scăzut de (...)
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  34. Epistemologia relativității generale.Nicolae Sfetcu - manuscript
    Empirismul logic al filosofiei științei a apărut în cea mai mare parte ca urmare a celor două teorii ale relativității lui Einstein, favorizând convenționalismul à la Poincaré față de neo-kantianism și pozitivismul machian. Filosofia empirismului logic al științei în sine se consideră că a fost formată din învățăturile extrase din teoria relativității. Câteva dintre cele mai caracteristice doctrine ale acestei filosofii (interpretarea elementelor a priori în teoriile fizice ca niște convenții, tratarea rolului necesar al convențiilor în dezvoltarea conceptelor teoretice din (...)
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  35. Ontologia singularităților gravitaționale.Nicolae Sfetcu - manuscript
    Relativitatea generală permite singularități. Trebuie să înțelegem ontologia singularităților gravitaționale dacă vrem să înțelegem natura spațiului și a timpului în universul actual. Deșii unii fizicieni consideră că singularitățile indică un eșec al relativității generale, alții cred că singularitățile deschid în fapt un orizont nou în cosmologie, cu fenomene fizice reale care pot ajuta la un progres profund în înțelegerea noastră a lumii. DOI: 10.13140/RG.2.2.31766.50242.
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  36. The Ontology of General Relativity.Nicolae Sfetcu - manuscript
    General Relativity generated various early philosophical interpretations. His adherents have highlighted the "relativization of inertia" and the concept of simultaneity, Kantians and Neo-Kantians have underlined the approach of certain synthetic "intellectual forms" (especially the principle of general covariance, and logical empirics have emphasized the philosophical methodological significance of the theory. Reichenbach approached the GR through the "relativity of geometry" thesis, trying to build a "constructive axiomatization" of relativity based on "elementary matters of fact" (Elementartatbestande) for the observable behavior of light (...)
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  37. Anomalies of General Relativity.Nicolae Sfetcu - manuscript
    Over time, the general theory of relativity has accumulated several anomalies and discrepancies, indicating the need for a better theory about gravity or other approaches. The ad-hoc hypotheses introduced in general relativity to explain gravitational singularities based on energy conditions are not very efficient. More detailed assumptions on the content of the subject are needed. Many scientists and philosophers have come to the conclusion that singularities must be associated with reaching the limits of the physical validity of general relativity, and (...)
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  38. Les singularités comme limites ontologiques de la relativité générale.Nicolae Sfetcu - manuscript
    Les singularités de la relativité générale résultant de la résolution des équations d'Einstein ont été et font encore l'objet de nombreux débats scientifiques : existe-t-il des singularités dans l'espace-temps ou pas ? Big Bang a été une singularité initiale ? Si les singularités existent, quelle est leur ontologie ? La théorie générale de la relativité est-elle une théorie qui a montré ses limites dans ce cas ? Dans cet essai, je soutiens qu'il existe des singularités et que la théorie de (...)
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  39. Tests classiques et modernes de la relativité générale.Nicolae Sfetcu - manuscript
    Albert Einstein a proposé trois tests de relativité générale, appelés plus tard les tests classiques de relativité générale, en 1916 : la précession de l'orbite de Mercure, la déviation de la lumière du soleil, et le décalage vers le rouge gravitationnel de la lumière. Dicke et Schiff ont établi un cadre pour tester la relativité générale , y compris par le biais d'expériences nulles et en utilisant la physique de l'exploration spatiale, de l'électronique et de la matière condensée, comme l'expérience (...)
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  40. Euristica relativității generale.Nicolae Sfetcu - manuscript
    Principiul esențial de coordonare în teoria generală a relativității este principiul echivalenței, incluzând o euristică negativă în conformitate cu metodologia programelor științifice de cercetare a lui Imre Lakatos. Argumentul ”nu este acela că toate cadrele de referință sunt echivalente, ci că coordonarea clasică a mișcării uniforme în linie dreaptă cu căile particulelor fără forță aplicată nu poate fi realizată fără nicio ambiguitate sau inconssistență.” Principiul echivalenței afirmă că descompunerea mișcării gravitaționale într-o mișcare uniformă și o accelerație gravitațională nu poate fi (...)
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  41. Épistémologie de la relativité générale.Nicolae Sfetcu - manuscript
    Les premières interprétations philosophiques de la théorie de la relativité générale sont très diverses, chacune essayant d'identifier Einstein comme un adepte de cette philosophie. Les partisans de Mach ont souligné la tentative d'Einstein de mettre en œuvre une « relativisation de l'inertie » dans la théorie générale, et son approche opérationnaliste de la simultanéité. Les kantiens et les néo-kantiens ont montré l'importance des « formes intellectuelles » synthétiques dans la théorie générale, en particulier le principe de covariance générale. Les empiristes (...)
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  42. Tests proposés par Einstein et des théories post-einsteiniennes.Nicolae Sfetcu - manuscript
    Einstein déclare que les théories évoluent à travers des déclarations basées sur l'observation, sous la forme de lois empiriques, à partir desquelles des lois générales sont obtenues. L'intuition et la pensée déductive jouent un rôle important dans ce processus. Après la phase initiale, l'investigateur développe un système de pensée guidée par des données empiriques, construit logiquement à partir d'hypothèses fondamentales (axiomes). La « vérité » d'une théorie résulte de sa corrélation avec un grand nombre d'observations uniques. Pour les mêmes données (...)
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  43. Classic Gravitational Tests of Post-Einsteinian Theories.Nicolae Sfetcu - manuscript
    Albert Einstein proposed three tests of general relativity, later named the classic tests of general relativity, in 1916: the precession of the perihelion of Mercury's orbit, sun light deflection, and the gravitational redshift of the light. For gravitational testing, the indirect effects of gravity are always used, usually particles that are influenced by gravity. In the presence of gravity, the particles move along curved geodesic lines. The sources of gravity that cause the curvature of spacetime are material bodies, depending on (...)
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  44. Teste clasice și moderne ale teoriilor relativiste ale gravitației.Nicolae Sfetcu - manuscript
    Cu ajutorul formalismului PPN se confruntă teoriile gravitației cu rezultatele experimentelor din sistemul solar. Parametrul γ din acest formalism evidențiază deformarea luminii și întârzierea luminii. Prin calcule în conformitate cu PPN se obține deformarea luminii în raport cu liniile drepte locale, comparativ cu tije rigide; din cauza curburii spațiului în jurul Soarelui, determinată de parametrul γ, liniile locale drepte sunt îndoite în raport cu liniile drepte asimptotice departe de Soare. Dezvoltarea interferometriei radio de bază foarte lungi (VLBI) a îmbunătățit măsurarea (...)
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  45. Gravitația newtoniană și relativistă.Nicolae Sfetcu - manuscript
    Gravitația clasică newtoniană admite o descriere geometrică. Împreună cu relativitatea specială, aceasta permite o descriere euristică a teoriei relativității generale. Mișcarea inerțială din mecanica clasică este legată de geometria spațiului și timpului, practic de-a lungul unor geodezice în care liniile de univers sunt linii drepte în spațiu-timpul relativist. Conform relativității generale, forţa de gravitaţie este o manifestare a geometriei locale spaţiu-timp. Relativitatea generală este o teorie metrică a gravitației. La baza ei sunt ecuațiile lui Einstein, care descriu relația dintre geometria (...)
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  46. Singularitățile ca limite ontologice ale relativității generale.Nicolae Sfetcu - manuscript
    Singularitățile la care se ajunge în relativitatea generală prin rezolvarea ecuațiilor lui Einstein au fost și încă mai sunt subiectul a numeroase dezbateri științifice: Există sau nu, singularități? Big Bang a fost o singularitate inițială? Dacă singularitățile există, care este ontologia acestora? Este teoria generală a relativității o teorie care și-a arătat limitele în acest caz? În acest eseu argumentez faptul că există singularități, iar teoria generală a relativității, ca de altfel oricare altă teorie științifică din prezent, nu este valabilă (...)
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  47. The Singularities as Ontological Limits of the General Relativity.Nicolae Sfetcu - manuscript
    The singularities from the general relativity resulting by solving Einstein's equations were and still are the subject of many scientific debates: Are there singularities in spacetime, or not? Big Bang was an initial singularity? If singularities exist, what is their ontology? Is the general theory of relativity a theory that has shown its limits in this case? In this essay I argue that there are singularities, and the general theory of relativity, as any other scientific theory at present, is not (...)
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  48. Classical Theory of Singularities.Nicolae Sfetcu - manuscript
    The singularities from the general relativity resulting by solving Einstein's equations were and still are the subject of many scientific debates: Are there singularities in spacetime, or not? Big Bang was an initial singularity? If singularities exist, what is their ontology? Is the general theory of relativity a theory that has shown its limits in this case?
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  49. Modern Tests of Relativistic Gravitational Theories.Nicolae Sfetcu - manuscript
    Dicke and Schiff established a framework for testing general relativity, including through null experiments and using the physics of space exploration, electronics and condensed matter, such as the Pound-Rebka experiment and laser interferometry. The gravitational lens tests and the temporal delay of light are highlighted by parameter γ of the PPN formalism, equal to 1 for general relativity and with different values in other theories. The BepiColombo mission aims to test the general theory of relativity by measuring the gamma and (...)
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  50. Tests de la relativité générale et des théories post-einsteiniennes.Nicolae Sfetcu - manuscript
    Au milieu des années 1970, de nombreuses théories alternatives de la gravité ont été confirmées par des expériences au niveau du système solaire, mais pas au niveau cosmologique. En 1974, Joseph Taylor et Russell Hulse ont découvert le pulsar binaire , dont les impulsions extrêmement stables ont été surveillées par radiotélescope, permettant une mesure précise des paramètres astrophysiques. En 1978, le taux de changement de la période orbitale du système a été mesuré, ce qui a été confirmé par la relativité (...)
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