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Scientific Contacts of Polish Physicists with Albert Einstein
The Global and the Local: The History of Science and the Cultural Integration of Europe. nd Proceedings of the 2 ICESHS (Cracow, Poland, September 6–9, 2006) / Ed. by M. Kokowski. Bronisław Średniawa * Scientific contacts of Polish physicists with Albert Einstein Abstract Scientific relations of Polish physicists, living in Poland and on emigration,with Albert Einstein, in the first half of 20th century are presented. Two Polish physicists, J. Laub and L. Infeld, were Einstein’s collaborators. The exchange of letters between M. Smoluchowski and Einstein contributed essentially to the solution of the problem of density fluctuations. S Loria, J. Kowalski, W. Natanson, M. Wolfke and L. Silberstein led scientific discussions with Einstein. Marie Skłodowska-Curie collaborated with Einstein in the Commission of Intelectual Cooperation of the Ligue of Nations. Einstein proposed scientific collaboration to M. Mathisson, but because of the breakout of the 2nd World War and Mathisson’s death their collaboration could not be realised. Contacts of Polish physicists with Einstein contributed to the development of relativity in Poland. (1) Introduction Many Polish physicists of older generation, who were active in Polish universities and abroad before the First World War or in the interwar period, had personal contacts with Einstein or exchanged letters with him. Contacts of Polish physicists with Einstein certainly inspired some Polish theoreticians to scientific work in relativity. These contacts encouraged also Polish physicists to make effort in the domain of popularization of relativity and of the progress of physics in the twenties and thirties. We can therefore say that the contacts of Polish physicists with Einstein contributed to the development of theoretical physics in Poland. -
The Son of Lamoraal Ulbo De Sitter, a Judge, and Catharine Theodore Wilhelmine Bertling
558 BIOGRAPHIES v.i WiLLEM DE SITTER viT 1872-1934 De Sitter was bom on 6 May 1872 in Sneek (province of Friesland), the son of Lamoraal Ulbo de Sitter, a judge, and Catharine Theodore Wilhelmine Bertling. His father became presiding judge of the court in Arnhem, and that is where De Sitter attended gymna sium. At the University of Groniiigen he first studied mathematics and physics and then switched to astronomy under Jacobus Kapteyn. De Sitter spent two years observing and studying under David Gill at the Cape Obsen'atory, the obseivatory with which Kapteyn was co operating on the Cape Photographic Durchmusterung. De Sitter participated in the program to make precise measurements of the positions of the Galilean moons of Jupiter, using a heliometer. In 1901 he received his doctorate under Kapteyn on a dissertation on Jupiter's satellites: Discussion of Heliometer Observations of Jupiter's Satel lites. De Sitter remained at Groningen as an assistant to Kapteyn in the astronomical laboratory, until 1909, when he was appointed to the chair of astronomy at the University of Leiden. In 1919 he be came director of the Leiden Observatory. He remained in these posts until his death in 1934. De Sitter's work was highly mathematical. With his work on Jupi ter's satellites, De Sitter pursued the new methods of celestial me chanics of Poincare and Tisserand. His earlier heliometer meas urements were later supplemented by photographic measurements made at the Cape, Johannesburg, Pulkowa, Greenwich, and Leiden. De Sitter's final results on this subject were published as 'New Math ematical Theory of Jupiter's Satellites' in 1925. -
The Big-Bang Theory AST-101, Ast-117, AST-602
AST-101, Ast-117, AST-602 The Big-Bang theory Luis Anchordoqui Thursday, November 21, 19 1 17.1 The Expanding Universe! Last class.... Thursday, November 21, 19 2 Hubbles Law v = Ho × d Velocity of Hubbles Recession Distance Constant (Mpc) (Doppler Shift) (km/sec/Mpc) (km/sec) velocity Implies the Expansion of the Universe! distance Thursday, November 21, 19 3 The redshift of a Galaxy is: A. The rate at which a Galaxy is expanding in size B. How much reader the galaxy appears when observed at large distances C. the speed at which a galaxy is orbiting around the Milky Way D. the relative speed of the redder stars in the galaxy with respect to the blues stars E. The recessional velocity of a galaxy, expressed as a fraction of the speed of light Thursday, November 21, 19 4 The redshift of a Galaxy is: A. The rate at which a Galaxy is expanding in size B. How much reader the galaxy appears when observed at large distances C. the speed at which a galaxy is orbiting around the Milky Way D. the relative speed of the redder stars in the galaxy with respect to the blues stars E. The recessional velocity of a galaxy, expressed as a fraction of the speed of light Thursday, November 21, 19 5 To a first approximation, a rough maximum age of the Universe can be estimated using which of the following? A. the age of the oldest open clusters B. 1/H0 the Hubble time C. the age of the Sun D. -
The Discovery of the Expansion of the Universe
galaxies Review The Discovery of the Expansion of the Universe Øyvind Grøn Faculty of Technology, Art and Design, Oslo Metropolitan University, PO Box 4 St. Olavs Plass, NO-0130 Oslo, Norway; [email protected]; Tel.: +047-90-94-64-60 Received: 2 November 2018; Accepted: 29 November 2018; Published: 3 December 2018 Abstract: Alexander Friedmann, Carl Wilhelm Wirtz, Vesto Slipher, Knut E. Lundmark, Willem de Sitter, Georges H. Lemaître, and Edwin Hubble all contributed to the discovery of the expansion of the universe. If only two persons are to be ranked as the most important ones for the general acceptance of the expansion of the universe, the historical evidence points at Lemaître and Hubble, and the proper answer to the question, “Who discovered the expansion of the universe?”, is Georges H. Lemaître. Keywords: cosmology history; expansion of the universe; Lemaitre; Hubble 1. Introduction The history of the discovery of the expansion of the universe is fascinating, and it has been thoroughly studied by several historians of science. (See, among others, the contributions to the conference Origins of the expanding universe [1]: 1912–1932). Here, I will present the main points of this important part of the history of the evolution of the modern picture of our world. 2. Einstein’s Static Universe Albert Einstein completed the general theory of relativity in December 1915, and the theory was presented in an impressive article [2] in May 1916. He applied [3] the theory to the construction of a relativistic model of the universe in 1917. At that time, it was commonly thought that the universe was static, since one had not observed any large scale motions of the stars. -
Einstein's Role in the Creation of Relativistic Cosmology
EINSTEIN'S ROLE IN THE CREATION OF RELATIVISTIC COSMOLOGY CHRISTOPHER SMEENK 1. Introduction Einstein's paper, \Cosmological Considerations in the General Theory of Relativ- ity" (Einstein 1917b), is rightly regarded as the first step in modern theoretical cosmology. Perhaps the most striking novelty introduced by Einstein was the very idea of a cosmological model, an exact solution to his new gravitational field equations that gives a global description of the universe in its entirety. Einstein's paper inspired a small group of theorists to study cosmological models using his new gravitational theory, and the ideas developed during these early days have been a crucial part of cosmology ever since. We will see below that understanding the physical properties of these models and their possible connections to astro- nomical observations was the central problem facing relativistic cosmology in the 20s. By the early 30s, there was widespread consensus that a class of models de- scribing the expanding universe was in at least rough agreement with astronomical observations. But this achievement was certainly not what Einstein had in mind in introducing the first cosmological model. Einstein's seminal paper was not simply a straightforward application of his new theory to an area where one would ex- pect the greatest differences from Newtonian theory. Instead, Einstein's foray into cosmology was a final attempt to guarantee that a version of \Mach's principle" holds. The Machian idea that inertia is due only to matter shaped Einstein's work on a new theory of gravity, but he soon realized that this might not hold in his “final” theory of November 1915. -
Appendix a the Return of a Static Universe and the End of Cosmology
Appendix A The Return of a Static Universe and the End of Cosmology Lawrence M. Krauss and Robert J. Scherrer Abstract We demonstrate that as we extrapolate the current CDM universe forward in time, all evidence of the Hubble expansion will disappear, so that observers in our “island universe” will be fundamentally incapable of determining the true nature of the universe, including the existence of the highly dominant vacuum energy, the existence of the CMB, and the primordial origin of light elements. With these pillars of the modern Big Bang gone, this epoch will mark the end of cosmology and the return of a static universe. In this sense, the coordinate system appropriate for future observers will perhaps fittingly resemble the static coordinate system in which the de Sitter universe was first presented. Shortly after Einstein’s development of general relativity, the Dutch astronomer Willem de Sitter proposed a static model of the universe containing no matter, which he thought might be a reasonable approximation to our low-density uni- verse. One can define a coordinate system in which the de Sitter metric takes a static form by defining de Sitter spacetime with a cosmological constant ƒ S W A B D 2 2 D 1 as a four-dimensional hyperboloid ƒ AB R ;R 3ƒ em- 2 D A B D bedded in a 5d Minkowski spacetime with ds AB d d ; and .AB / diag.1; 1; 1; 1; 1/;A;B D 0;:::;4: The static form of the de Sitter metric is then dr2 ds2 D .1 r2=R2/dt 2 s r2d2; s s s 2 2 s 1 rs =R L.M. -
The Experimental Verdict on Spacetime from Gravity Probe B
The Experimental Verdict on Spacetime from Gravity Probe B James Overduin Abstract Concepts of space and time have been closely connected with matter since the time of the ancient Greeks. The history of these ideas is briefly reviewed, focusing on the debate between “absolute” and “relational” views of space and time and their influence on Einstein’s theory of general relativity, as formulated in the language of four-dimensional spacetime by Minkowski in 1908. After a brief detour through Minkowski’s modern-day legacy in higher dimensions, an overview is given of the current experimental status of general relativity. Gravity Probe B is the first test of this theory to focus on spin, and the first to produce direct and unambiguous detections of the geodetic effect (warped spacetime tugs on a spin- ning gyroscope) and the frame-dragging effect (the spinning earth pulls spacetime around with it). These effects have important implications for astrophysics, cosmol- ogy and the origin of inertia. Philosophically, they might also be viewed as tests of the propositions that spacetime acts on matter (geodetic effect) and that matter acts back on spacetime (frame-dragging effect). 1 Space and Time Before Minkowski The Stoic philosopher Zeno of Elea, author of Zeno’s paradoxes (c. 490-430 BCE), is said to have held that space and time were unreal since they could neither act nor be acted upon by matter [1]. This is perhaps the earliest version of the relational view of space and time, a view whose philosophical fortunes have waxed and waned with the centuries, but which has exercised enormous influence on physics. -
Hubble's Diagram and Cosmic Expansion
Hubble’s diagram and cosmic expansion Robert P. Kirshner* Harvard–Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 Contributed by Robert P. Kirshner, October 21, 2003 Edwin Hubble’s classic article on the expanding universe appeared in PNAS in 1929 [Hubble, E. P. (1929) Proc. Natl. Acad. Sci. USA 15, 168–173]. The chief result, that a galaxy’s distance is proportional to its redshift, is so well known and so deeply embedded into the language of astronomy through the Hubble diagram, the Hubble constant, Hubble’s Law, and the Hubble time, that the article itself is rarely referenced. Even though Hubble’s distances have a large systematic error, Hubble’s velocities come chiefly from Vesto Melvin Slipher, and the interpretation in terms of the de Sitter effect is out of the mainstream of modern cosmology, this article opened the way to investigation of the expanding, evolving, and accelerating universe that engages today’s burgeoning field of cosmology. he publication of Edwin Hub- ble’s 1929 article ‘‘A relation between distance and radial T velocity among extra-galactic nebulae’’ marked a turning point in un- derstanding the universe. In this brief report, Hubble laid out the evidence for one of the great discoveries in 20th cen- tury science: the expanding universe. Hubble showed that galaxies recede from us in all directions and more dis- tant ones recede more rapidly in pro- portion to their distance. His graph of velocity against distance (Fig. 1) is the original Hubble diagram; the equation that describes the linear fit, velocity ϭ ϫ Ho distance, is Hubble’s Law; the slope of that line is the Hubble con- ͞ stant, Ho; and 1 Ho is the Hubble time. -
Space, Time, and Spacetime
Fundamental Theories of Physics 167 Space, Time, and Spacetime Physical and Philosophical Implications of Minkowski's Unification of Space and Time Bearbeitet von Vesselin Petkov 1. Auflage 2010. Buch. xii, 314 S. Hardcover ISBN 978 3 642 13537 8 Format (B x L): 15,5 x 23,5 cm Gewicht: 714 g Weitere Fachgebiete > Physik, Astronomie > Quantenphysik > Relativität, Gravitation Zu Inhaltsverzeichnis schnell und portofrei erhältlich bei Die Online-Fachbuchhandlung beck-shop.de ist spezialisiert auf Fachbücher, insbesondere Recht, Steuern und Wirtschaft. Im Sortiment finden Sie alle Medien (Bücher, Zeitschriften, CDs, eBooks, etc.) aller Verlage. Ergänzt wird das Programm durch Services wie Neuerscheinungsdienst oder Zusammenstellungen von Büchern zu Sonderpreisen. Der Shop führt mehr als 8 Millionen Produkte. The Experimental Verdict on Spacetime from Gravity Probe B James Overduin Abstract Concepts of space and time have been closely connected with matter since the time of the ancient Greeks. The history of these ideas is briefly reviewed, focusing on the debate between “absolute” and “relational” views of space and time and their influence on Einstein’s theory of general relativity, as formulated in the language of four-dimensional spacetime by Minkowski in 1908. After a brief detour through Minkowski’s modern-day legacy in higher dimensions, an overview is given of the current experimental status of general relativity. Gravity Probe B is the first test of this theory to focus on spin, and the first to produce direct and unambiguous detections of the geodetic effect (warped spacetime tugs on a spin- ning gyroscope) and the frame-dragging effect (the spinning earth pulls spacetime around with it). -
Fqxi 4Dave Last1-3-9-Kor Ende
! Revising Space Time Geometry: A Proposal for a New Romance in Many Dimensions Renate Quehenberger* Quantum Cinema - a digital Vision (PEEK) Department of Mediatheory at the University of Applied Arts, Vienna August 25, 2012 Abstract The ontological positioning of our existence, deeply connected with the hierarchy problem concerning the dimensions of space and time, is one of the major problems for our understanding of the “ultimate” nature of reality. The resulting problem is that mathematical concepts that need so-called “extra-dimensions” have been widely disregarded owing to a lack of physical interpretation. This article reviews conventions, imaginations and assumptions about the non-imaginative by starting at the origins of the of 4D and 5D space-time concepts and proposing a new geometrical approach via a hyper- Euclidian path for a mentally accessible vision of continuous AND discrete complex space configuration in dimensions up to higher order. e-mail address: [email protected] 1 RCZ Quehenberger “Time and Space... It is not nature which imposes them upon us, it is we who impose them upon nature because we find them convenient.” [Henri Poincaré, 1905] Introduction The general physicists’ assertion is that we are living in a three-dimensional world with one time- dimension and cosmic space is curved in the fourth dimension is based on a relativistic world view that has gained general acceptance. In fact this is a post-Copernicanian world view which does not pay attention to the consequences of Max Planck’s revolution and the development in quantum physics of the past 100 years. -
Einstein's Conversion from His Static to an Expanding Universe
Eur. Phys. J. H DOI: 10.1140/epjh/e2013-40037-6 THE EUROPEAN PHYSICAL JOURNAL H Einstein’s conversion from his static to an expanding universe Harry Nussbaumera Institute of Astronomy, ETH Zurich, CH-8093 Zurich, Switzerland Received 19 September 2013 / Received in final form 13 November 2013 Published online 4 February 2014 c EDP Sciences, Springer-Verlag 2014 Abstract. In 1917 Einstein initiated modern cosmology by postulating, based on general relativity, a homogenous, static, spatially curved uni- verse. To counteract gravitational contraction he introduced the cos- mological constant. In 1922 Alexander Friedman showed that Albert Einstein’s fundamental equations also allow dynamical worlds, and in 1927 Georges Lemaˆıtre, backed by observational evidence, con- cluded that our universe was expanding. Einstein impetuously rejected Friedman’s as well as Lemaˆıtre’s findings. However, in 1931 he retracted his former static model in favour of a dynamic solution. This investiga- tion follows Einstein on his hesitating path from a static to the expand- ing universe. Contrary to an often advocated belief the primary motive for his switch was not observational evidence, but the realisation that his static model was unstable. 1 Introduction It has become a popular belief that Albert Einstein abandoned his static universe when, on a visit to Pasadena in January and February 1931, Edwin Hubble showed him the redshifted nebular spectra and convinced him that the universe was expand- ing, and the cosmological constant was superfluous. “Two months with Hubble were enough to pry him loose from his attachment to the cosmological constant” is just one example of such statements [Topper 2013]. -
Simulating Galactical Vorticity Using a Supersymmetric Operator
See discussions, stats, and author profiles for this publication at: https://www.researchgate.net/publication/340262362 Simulating galactical vorticity using a supersymmetric operator Technical Report · March 2020 DOI: 10.13140/RG.2.2.34254.00323 CITATIONS READS 0 16 2 authors: Sergio Manzetti Alexander Trunev Fjordforsk A/S Likalo LLC, Toronto, Canada 107 PUBLICATIONS 1,125 CITATIONS 101 PUBLICATIONS 109 CITATIONS SEE PROFILE SEE PROFILE Some of the authors of this publication are also working on these related projects: Halogenated silica nanoparticles for solar cell technologies. View project Wavefunction studies of molecules and oligomers. View project All content following this page was uploaded by Sergio Manzetti on 29 March 2020. The user has requested enhancement of the downloaded file. Simulating galactical vorticity using a supersymmetric operator. Sergio Manzetti 1;2∗ and Alexander Trounev 1;3 1. Fjordforsk A/S, Midtun, 6894 Vangsnes, Norway. Email: [email protected] 2.Uppsala University, BMC, Dept Mol. Cell Biol, Box 596, SE-75124 Uppsala, Sweden. 3. A & E Trounev IT Consulting, Toronto, Canada. March 29, 2020 1 Abstract 1 Simulations of galactic vorticity require the development of complex systems of equations to generate models that account for the gravity, mass, kinetic, and electromagnetic effects which govern cluster behaviour. In this study, a rela- tionship is outlined through a series of steps, between the Einstein equations, the Ricci equations and the gravitational model of comoslogical bodies. This series of steps are then followed by the generation of a group of equations, in- cluding a supersymmetric equation which describes vorticity under the presence of an electromagnetic field for quantized systems.