Minimal Energy and Gravitation     

Corrado Massa 《Astrophysics and Space Science》2006,305(4):377-384

Quantum theory in Robertson – Walker spacetime suggests the existence of a minimal energy ε of the order of 10⁻⁴⁵ erg. Reasonable forms for ε give the expansion factor R=R(t)(t= the cosmic time) with no need of gravitational field equations.Einstein's theory should be modified in gravitational fields of strength less than ε c/ħ ∼ 10⁻⁸ cm/s² where c is the speed of light and ħ is the reduced Planck constant. The cosmological term λ is expected to decrease as the universe expands.In the Appendix, ε is derived from a big bang – big crunch Newtonian cosmology.  相似文献   

Can the bump in the composite spectrum of GRB 910503 be an emission line feature of gamma-ray bursts？     

Yi-Ping Qin  Pu-Wen Zhang National Astronomical Observatories  Yunnan Observatory  Chinese Academy  of Sciences  Kunming Physics Department  Guangxi University  Nanning Graduate University of Chinese Academy of Sciences  Beijing 《中国天文和天体物理学报》2005,5(6):627-635

Appearing in the composite spectral data of BATSE, EGRET and COMPTEL for GRB 910503, there is a bump at around 1600 keV. We perform a statistical analysis on the spectral data, trying to find out if the bump could be accounted for by a blue-shifted and significantly broadened rest frame line due to the Doppler effect of an expanding fireball surface. We made an F-test and adopted previously proposed criteria. The study reveals that the criteria are well satisfied and the feature can be interpreted as the blue shifted 6.4 keV line. Prom the fit with this line taken into account, we find the Lorentz factor of this source to be P = 116-9+9 (at the 68% confident level,△x2 = 1) and the rest frame spectral peak energy to be E0,p- 2.96-0.18+0.24 keV. Although the existence of the emission line feature requires other independent tests to confirm, the analysis suggests that it is feasible to detect emission line features in the high energy range of GRB spectra when taking into account the Doppler effect of fireball expansion.  相似文献   

Iron line profiles in strong gravity     

Kris Beckwith  Chris Done 《Monthly notices of the Royal Astronomical Society》2004,352(2):353-362

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On Relativistic Equations of Motion of an Earth Satellite     

V. A. Brumberg 《Celestial Mechanics and Dynamical Astronomy》2004,88(2):209-225

For numerical integration of the geocentric equations of motion of Earth satellites in the general relativity framework one may choose now between rather simple equations involving in their relativistic dynamical part only the Earth-induced terms and very complicated equations taking into account the relativistic third-body action. However, it is possible quite easily to take into account the relativistic indirect third-body perturbations and to neglect much lesser direct third-body perturbations. Such approach is based on the use of the Newtonian third-body perturbations in geocentric variables with expressing them in the relativistic manner in terms of the barycentric arguments. Together with it, to extend the known results for the spheroid model of the Earth, the Earth-induced terms are treated in great detail by including the non-spin part of the Earth vector-potential and the Earth triaxial non-sphericity.This revised version was published online in October 2005 with corrections to the Cover Date.  相似文献   

语言相对性与英语的区域性变体研究   总被引：1，自引：0，他引：1  

郭遂红 《广东海洋大学学报》2004,24(5):64-69

英语已发展成为一门世界性语言 ,英语在非英语国家的发展已经形成了许多带有浓厚地域特色的变体。从语言相对性的角度对英语区域性变体进行分析研究 ,论述其产生的历史根源是由于英国在世界上的扩张、以及文化差异 ,并阐述了英语区域性变体的分类以及人们对区域性变体所持的态度。  相似文献   

Creation of electron–positron wind in gamma-ray bursts and its effect on the early afterglow emission     

P. Kumar  A. Panaitescu 《Monthly notices of the Royal Astronomical Society》2004,354(1):252-258

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Non-linear pulsations in differentially rotating neutron stars: mass-shedding-induced damping and splitting of the fundamental mode     

Nikolaos Stergioulas  Theocharis A. Apostolatos  José A. Font 《Monthly notices of the Royal Astronomical Society》2004,352(4):1089-1101

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Describing neutron stars by the relativistic mean field theory     

Huan-yu Jia  Bao-xi Sun  Jie Meng  En-guang Zhao 《Chinese Astronomy and Astrophysics》2002,26(4):901-413

Neutron stars are studied in the framework of the relativistic mean field theory of interacting nucleons, hyperons, and mesons. Within the hadronic freedom, the cores of neutron stars are found to be dominated by hyperons when the density is sufficiently high. The influence of hyperon coupling constants on the transition from a neutron star to a hyperon-dominated strange neutron star is also investigated. It is found that the transition density gets its minimum value when the ratio of hyperon coupling constant to nucleon's takes the value of 0.65, and the calculated maximum mass of the neutron star is 1.4 M which lies within the range of the observational results.  相似文献   

最新规范的参考系及有关问题     

潘炼德 《时间频率学报》2002,25(2):131-140

在简要阐明参考系、参考架及其历史重大进程的基础上,对几种重要的、最新规范的参考系/参考架(质心天球参考系和地心天球参考系、国际天球参考系、国际地球参考系、太阳系动力学参考系等)的定义、实现和特点作了评述和分析,并对最新规范中与参考系、参考架有关的某些新概念的定义和新模式的应用(自2003年开始贯彻),如:天球中介极(CIP)、天球历书原点(CEO)、地球历书原点(TEO)、地球自转角的新定义、岁差-章动新模式的应用,作了阐述和讨论。  相似文献   

相对论天体力学和后牛顿运动方程     

易照华 《天文研究与技术》2002,(3):9-16

叙述了与Astrod工程有关的相对论天体力学基础内容。包括相对论天体力学、广义相对论基本原理、PPN方法体系、PPN多体问题、PPN二体问题。高阶PN二体问题等  相似文献