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1.Cosmic Expansion and Cosmological Distances
2.A different physical interpretation on the cosmic expansion agent
宇宙膨胀动因的另类物理解释收藏指正
3.HIGHz Ⅰ a SUPERNOVAE SEARCH AND THE ACCELERATION OF THE COSMIC EXPANSION
高红移Ⅰ_a型超新星的搜寻和宇宙的加速膨胀收藏指正
4.Cosmic expansion has got its groove back: once thought to be winding down, it is actually speeding up.
宇宙膨胀也因此重获律动:当你认为它应该变慢时,实际上却变快了。收藏指正
5.Like Darwinian evolution, cosmic expansion provides the context within which simple structures form and develop over time into complex structures.
宇宙膨胀就像达尔文的演化论,对于简单的结构如何逐步发展形成复杂的结构,提供了可循的脉络。收藏指正
6.Cosmic expansion had diluted the density of the gas to the point where collisions were too infrequent to equalize the spin and kinetic temperatures.
宇宙膨胀至此,已将气体稀释到一定的程度,使得原子碰撞不再频繁地让自旋与动力温度相等。收藏指正
7.You will probably die long before your alter egos come into view, but in principle, and if cosmic expansion cooperates, your descendants could observe them through a sufficiently powerful telescope.
也许你早在见到另一个你的很久以前就死了,但是原则上,如果宇宙膨胀的方式肯配合,有一天你的后代子孙,应该可以用够强的望远镜观察到他们。收藏指正
8.Topics include: planets, planet formation; stars, the Sun, "normal" stars, star formation; stellar evolution, supernovae, compact objects (white dwarfs, neutron stars, and black holes), plusars, binary X-ray sources; star clusters, globular and open clusters; interstellar medium, gas, dust, magnetic fields, cosmic rays; distance ladder; galaxies, normal and active galaxies, jets; gravitational lensing; large scaling structure; Newtonian cosmology, dynamical expansion and thermal history of the Universe; cosmic microwave background radiation; big-bang nucleosynthesis.
课程的主题包含了:行星、行星形成;恒星、太阳、正常的恒星、恒星形成;恒星演化、超新星、致密天体(白矮星、中子星及黑洞)、波霎、双X-射线源;星团、球状及疏散星团;星际介质、气体、尘埃、磁场、宇宙射线;距离阶梯;星系、正常及活跃星系、喷流;重力透镜;大尺度结构;牛顿宇宙学、宇宙的动力膨胀及温度发展历史;宇宙背景微波辐射;大霹雳核合成。收藏指正
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