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In calculations of the probability distribution for the cosmological constant, it has been previously assumed that the a priori probability distribution is essentially constant in the very narrow range that is anthropically allowed. This…

天体物理学 · 物理学 2009-10-31 Steven Weinberg

We discuss the value of the cosmological constant as recovered from CMB and LSS data and the robustness of the results when general isocurvature initial conditions are allowed for, as opposed to purely adiabatic perturbations. The Bayesian…

天体物理学 · 物理学 2015-06-24 Roberto Trotta

Recent analyses of Brahmagupta's discourse on the cyclic quadrilateral, and of Baudh\=ayana's approximate quadrature of the circle, have shown that it is useful to submit mathematical texts to a form of literary analysis. Several passages…

历史与综述 · 数学 2025-07-08 Satyanad Kichenassamy

We develop a phenomenological theory that aims to account for the origin of the large eccentricities of extrasolar planets and that of the small eccentricities in the solar system, the preference for apsidal alignment in non-resonant…

天体物理学 · 物理学 2008-11-26 Fathi Namouni

The majority of star formation results in binaries or higher multiple systems, and planets in such systems are constrained to a limited range of orbital parameters in order to remain stable against perturbations from stellar companions.…

地球与行星天体物理 · 物理学 2024-07-22 Billy Quarles , Hareesh Gautham Bhaskar , Gongjie Li

This chapter discusses the dynamical properties of the Kuiper belt population. Then, it focuses on the characteristics of the Kuiper belt that cannot be explained by its evolution in the framework of the current solar system. We review…

天体物理学 · 物理学 2007-05-23 A. Morbidelli , H. F. Levison , R. Gomes

Starting from a previously stated hypothesis concerning the discretization of the orbits for periodic celestial motions, the mass of ups-Andromedae and the periods of its b- and d- companions are estimated using the accurately known period…

天体物理学 · 物理学 2007-05-23 A. G. Agnese , R. Festa

Supernovae observations strongly support the presence of a cosmological constant, but its value, which we will call apparent, is normally determined assuming that the universe can be accurately described by a homogeneous model. Even in the…

广义相对论与量子宇宙学 · 物理学 2012-11-07 Antonio Enea Romano , Pisin chen

This article presents a brief description of India's AstroSat mission which is a powerful space based observatory for compact star research. An account is given of observational constraints and spectral and timing capabilities as realised…

天体物理仪器与方法 · 物理学 2017-09-22 Dipankar Bhattacharya

We compute the expected value of the cosmological constant in our universe from the Causal Entropic Principle. Since observers must obey the laws of thermodynamics and causality, the principle asserts that physical parameters are most…

高能物理 - 理论 · 物理学 2008-11-26 Raphael Bousso , Roni Harnik , Graham D. Kribs , Gilad Perez

The causal entropic principle aims to predict the unexpectedly small value of the cosmological constant Lambda using a weighting by entropy increase on causal diamonds. The original work assumed a purely isotropic and homogeneous cosmology.…

广义相对论与量子宇宙学 · 物理学 2012-01-20 Daniel Phillips , Andreas Albrecht

The bright F8 V solar-type star upsilon Andromedae has recently been reported to have a system of three planets of Jovian masses. In order to investigate the orbital stability and mutual gravitational interactions among these extrasolar…

天体物理学 · 物理学 2009-10-31 Ing-Guey Jiang , Wing-Huen Ip

Recent astrophysical observations seem to indicate that the cosmological constant is small but nonzero and positive. The old cosmological constant problem asks why it is so small; we must now ask, in addition, why it is nonzero (and is in…

高能物理 - 理论 · 物理学 2011-04-15 Y. Jack Ng , H. van Dam

We evaluate the orbital evolution and several plausible origins scenarios for the mutually inclined orbits of Upsilon Andromedae c and d. These two planets have orbital elements that oscillate with large amplitudes and lie close to the…

地球与行星天体物理 · 物理学 2015-05-20 Rory Barnes , Richard Greenberg , Thomas R. Quinn , Barbara E. McArthur , G. Fritz Benedict

The common nature of dark matter and dark energy is argued in [1] based on the approach that the cosmological constant \Lambda enters the weak-field General Relativity following from Newton theorem on the "sphere-point mass" equivalency…

综合物理 · 物理学 2019-02-27 V. G. Gurzadyan , A. Stepanian

The difference in formation process between binary stars and planetary systems is reflected in their composition as well as their orbital architecture, particularly orbital eccentricity as a function of orbital period. It is suggested here…

天体物理学 · 物理学 2009-10-30 David C. Black

The basic geometry of the Solar System -- the shapes, spacings, and orientations of the planetary orbits -- has long been a subject of fascination as well as inspiration for planet formation theories. For exoplanetary systems, those same…

地球与行星天体物理 · 物理学 2015-10-19 Joshua N. Winn , Daniel C. Fabrycky

Planetary satellites are an integral part of the heirarchy of planetary systems. Here we make two predictions concerning their formation. First, primordial satellites, which have an array of distinguishing characteristics, form only around…

地球与行星天体物理 · 物理学 2012-04-05 Paul Withers , Jason W. Barnes

This is a historian's view of how modern astronomy data can be used to discuss the shifting historical worldview of Late Antiquity. In this article an attemp is made to construct an approximate model of how the cycles of astronomical…

物理学史与哲学 · 物理学 2024-03-07 D. N. Starostin

This chapter concerns the long-term dynamical evolution of planetary systems from both theoretical and observational perspectives. We begin by discussing the planet-planet interactions that take place within our own Solar System. We then…