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In 1892 H.A. Lorentz started the search for a classical equation of motion for pointlike charged particles that takes into account the radiation reaction force. This search culminated in the Lorentz-Abraham-Dirac equation of motion, which…

经典物理 · 物理学 2007-05-23 Marijan Ribaric , Luka Sustersic

Given a solar luminosity L_Ar = 0.75 L_0 at the beginning of the Archean 3.8 Gyr ago, where L_0 is the present-day one, if the heliocentric distance r of the Earth was r_Ar = 0.956 r_0, the solar irradiance would have been as large as I_Ar…

地球与行星天体物理 · 物理学 2013-10-21 Lorenzo Iorio

The herein presented analytical framework fully describes the motion of coplanar systems consisting of a stellar binary and a planet orbiting both stars on orbital as well as secular timescales. Perturbations of the Runge-Lenz vector are…

地球与行星天体物理 · 物理学 2015-06-24 Nikolaos Georgakarakos , Siegfried Eggl

We consider the Lorenz equations, a system of three dimensional ordinary differential equations modeling atmospheric convection. These equations are chaotic and hard to study even numerically, and so a simpler "geometric model" has been…

动力系统 · 数学 2024-05-14 Tali Pinsky

The inflationary hot big bang model of cosmology explains the birth of the universe, the appearance of atoms and that of large-scale structures, altogether omitting any reference to the living world. Yet, like the physical world, the living…

生物物理 · 物理学 2021-08-17 L. Wirtanen

The hodograph of the Kepler-Coulomb problem, that is, the path traced by its velocity vector, is shown to be a circle and then it is used to investigate other properties of the motion. We obtain the configuration space orbits of the problem…

The periodic orbit conjecture states that, on closed manifolds, the set of lengths of the orbits of a non-vanishing vector field all whose orbits are closed admits an upper bound. This conjecture is known to be false in general due to a…

动力系统 · 数学 2021-05-26 Robert Cardona

In 1936, Albert Einstein wrote a brief article where he suggested the possibility that a massive object acted as a lens, amplifying the brightness of a star. As time went by, this phenomenon, known as gravitational lensing, has become a…

科普物理 · 物理学 2018-08-01 Jorge Pinochet , Michael Van Sint Jan

The concept of dark matter in the Universe and its components has been discussed in the 1930s by several authors, and in particular by Oort (1932) and Zwicky (1933). However, it is only in the 1970s that the existence of dark matter was…

科普物理 · 物理学 2023-09-13 Albert Bosma

An attempt is made to explain the spiral structure of spiral galaxies through a possible rotation of the Universe. To this end, we write down a possible form of the metric, and we calculate the necessary quantities (Rik, Tik, ...) in order…

天体物理学 · 物理学 2009-04-27 Evangelos Chaliasos

Bohr's interpretation of quantum mechanics has been criticized as incoherent and opportunistic, and based on doubtful philosophical premises. If so Bohr's influence, in the pre-war period of 1927-1939, is the harder to explain, and the…

量子物理 · 物理学 2009-11-10 Simon Saunders

Standard solar models predict a solar luminosity that gradually increased by about 30% over the past 4.5 billion years. Under the faint sun, Earth should have been frozen solid for most of its existence. Yet, running water is observed to…

天体物理学 · 物理学 2015-06-24 Nir J. Shaviv

Most mechanisms proposed for the formation of planets are modified versions of the mechanism proposed for the solar system. Here we argue that, in terms of those planetary systems which have been observed, the case for the solar system…

天体物理学 · 物理学 2009-11-10 M. E. Beer , A. R. King , M. Livio , J. E. Pringle

The objective of this paper is not simply to present an historical overview of Einstein's cosmological considerations, but to discuss the central role they played in shaping the paradigm of relativistic cosmology. This, we'll show, was a…

物理学史与哲学 · 物理学 2014-02-14 Daryl Janzen

Between 1905 and 1907, Einstein first tried to extend the special theory of relativity in such a way so as to explain gravitational phenomena. This was the most natural and simplest path to be taken. These investigations did not fit in with…

物理学史与哲学 · 物理学 2012-08-28 Galina Weinstein

Large astronomical objects such as stars or planets, produce approximately spherical shapes due to the large gravitational forces, and if the object is rotating rapidly, it becomes an oblate spheroid. In juxtaposition to this, we conduct a…

经典物理 · 物理学 2012-06-19 James M. Chappell , Mark J. Chappell , Azhar Iqbal , Derek Abbott

Most of our knowledge about the Sun's activity cycle arises from sunspot observations over the last centuries since telescopes have been used for astronomy. The German astronomer Gustav Sp\"orer observed almost daily the Sun from 1861 until…

太阳与恒星天体物理 · 物理学 2015-11-11 Andrea Diercke , Rainer Arlt , Carsten Denker

The solar luminosity in the visible changes at the 10-3 level, following an 11 years period. In X-rays, which should not be there, the amplitude varies 100000 times stronger, making their mysterious origin since the discovery in 1938 even…

太阳与恒星天体物理 · 物理学 2015-06-17 K. Zioutas , M. Tsagri , Y. K. Semertzidis , T. Papaevangelou , D. H. H. Hoffmann , V. Anastassopoulos

Let m(i) be the mass of i-th planet and M be the Solar mass. From astronomical data it is known that ratios r(i)=m(i)/(m(i)+M) are of order 10^(-3)-10^(-6) for all planets. The same is true for all satellites of heavy planets. These results…

广义相对论与量子宇宙学 · 物理学 2011-03-28 Arkady L. Kholodenko

Almost half a century before Einstein expounded his general theory of relativity, the English mathematician William Kingdon Clifford argued that space might not be Euclidean and proposed that matter is nothing but a small distortion in that…

物理学史与哲学 · 物理学 2018-07-25 S. Galindo , Jorge L. Cervantes-Cota
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