標(biāo)題: Titlebook: Cosmology for the Curious; Delia Perlov,Alex Vilenkin Book 2024Latest edition The Editor(s) (if applicable) and The Author(s), under exclu [打印本頁] 作者: FLAW 時(shí)間: 2025-3-21 19:17
書目名稱Cosmology for the Curious影響因子(影響力)
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作者: 小樣他閑聊 時(shí)間: 2025-3-21 21:59 作者: BALE 時(shí)間: 2025-3-22 01:44 作者: MODE 時(shí)間: 2025-3-22 06:08 作者: 油氈 時(shí)間: 2025-3-22 08:52
Special Relativityng, as long as the motion was uniform (that is, at a constant speed) and in the same direction, without any turns. While the ship was the vehicle of choice in Galileo’s time, all of us can recall a similar experience in a train or an airplane. When the ride is smooth and you do not look outside, you cannot tell whether you are moving or not.作者: FILTH 時(shí)間: 2025-3-22 14:28 作者: FILTH 時(shí)間: 2025-3-22 20:12 作者: 不如屎殼郎 時(shí)間: 2025-3-22 23:39
https://doi.org/10.1007/978-94-017-8987-5e matter is uniformly distributed in the cosmos. There are of course local variations, with the density of stars higher in some places and lower in others. However on very large scales the universe is well approximated as being perfectly homogeneous.作者: lobster 時(shí)間: 2025-3-23 03:33 作者: persistence 時(shí)間: 2025-3-23 09:36 作者: 凝乳 時(shí)間: 2025-3-23 11:18 作者: Iniquitous 時(shí)間: 2025-3-23 15:44 作者: 開始從未 時(shí)間: 2025-3-23 18:26 作者: indigenous 時(shí)間: 2025-3-24 01:30 作者: 退潮 時(shí)間: 2025-3-24 03:04 作者: 因無茶而冷淡 時(shí)間: 2025-3-24 07:52 作者: Feckless 時(shí)間: 2025-3-24 12:51
A Historical Overview, using the language of modern physics and abstract mathematics. Yet, at its core, our cosmological knowledge is the answer to a few fundamental questions. Have you ever drifted off deep into thought, wondering: Is the universe finite or infinite? Has it existed forever? If not, when and how did it 作者: Felicitous 時(shí)間: 2025-3-24 18:56 作者: 業(yè)余愛好者 時(shí)間: 2025-3-24 21:07 作者: daredevil 時(shí)間: 2025-3-25 02:25
An Expanding Universeniverse beyond our Milky Way galaxy was then completely unknown, so Einstein had to make some assumptions. Following Newton, he assumed that on average matter is uniformly distributed in the cosmos. There are of course local variations, with the density of stars higher in some places and lower in ot作者: 半圓鑿 時(shí)間: 2025-3-25 05:20
Hubble’s Law and the Expanding Universeeriously had spectral lines that were red-shifted, indicating that they were moving away from the Earth, some at speeds of up to 1000?km/s. Motion at high speed is not uncommon in the cosmos—the Sun, for example, orbits around the center of our Galaxy at 240 km/s.作者: Moderate 時(shí)間: 2025-3-25 09:36
The Quantum Worlde, was single handedly accomplished by Einstein with his special and general theories of relativity. The development ofby a number of physicists ushered in the second revolution, which shook the foundations of physics even more than the first. Quantum mechanics was developed as a theory of the micro作者: effrontery 時(shí)間: 2025-3-25 15:27
The Hot Big Bangnd that the universe was denser in its past than it is today. In fact, the density of the universe grows without bound as we wind the clock back to the big bang. Furthermore, the temperature of the universe also soars to extremely high values. How do we know this? And what does this imply about the 作者: 使長胖 時(shí)間: 2025-3-25 18:44
Structure Formations are grouped in clusters, which are in turn grouped into still larger structures, called superclusters. The formation of cosmic structures is an active area of research, and we now believe we have a good idea of how they emerged.作者: Middle-Ear 時(shí)間: 2025-3-25 21:30 作者: 懸崖 時(shí)間: 2025-3-26 04:09
The Very Early Universebang, the fireball gets hotter and denser, and other types of particles emerge. They move at nearly the speed of light, colliding frequently and violently. As we shall see, some of the most dramatic events in the history of the universe occurred within a small fraction of a second after the big bang作者: 啞巴 時(shí)間: 2025-3-26 06:10
A Test Bed for the Numerical Tool, using the language of modern physics and abstract mathematics. Yet, at its core, our cosmological knowledge is the answer to a few fundamental questions. Have you ever drifted off deep into thought, wondering: Is the universe finite or infinite? Has it existed forever? If not, when and how did it 作者: tinnitus 時(shí)間: 2025-3-26 11:34 作者: 粘連 時(shí)間: 2025-3-26 13:24
Shuzhuo Li,Quanbao Jiang,Marcus W. Feldmanatible with Newton’s law of gravitation. Newton himself, and some ten generations of physicists and astronomers that followed, used this law to describe the motion of planets with remarkable accuracy. Granted, there was a tiny discrepancy in the calculated precession rate of the orbit of Mercury, bu作者: Protein 時(shí)間: 2025-3-26 18:48
https://doi.org/10.1007/978-94-017-8987-5niverse beyond our Milky Way galaxy was then completely unknown, so Einstein had to make some assumptions. Following Newton, he assumed that on average matter is uniformly distributed in the cosmos. There are of course local variations, with the density of stars higher in some places and lower in ot作者: nonradioactive 時(shí)間: 2025-3-26 21:26 作者: concentrate 時(shí)間: 2025-3-27 01:11 作者: nascent 時(shí)間: 2025-3-27 06:01 作者: osculate 時(shí)間: 2025-3-27 11:34
https://doi.org/10.1007/978-3-030-85574-1s are grouped in clusters, which are in turn grouped into still larger structures, called superclusters. The formation of cosmic structures is an active area of research, and we now believe we have a good idea of how they emerged.作者: WAX 時(shí)間: 2025-3-27 16:50 作者: 你敢命令 時(shí)間: 2025-3-27 19:15
Valeria Minghetti,Federica Montagutibang, the fireball gets hotter and denser, and other types of particles emerge. They move at nearly the speed of light, colliding frequently and violently. As we shall see, some of the most dramatic events in the history of the universe occurred within a small fraction of a second after the big bang作者: 按時(shí)間順序 時(shí)間: 2025-3-28 01:08 作者: guardianship 時(shí)間: 2025-3-28 04:29 作者: 殘忍 時(shí)間: 2025-3-28 06:50
Hubble’s Law and the Expanding Universeeriously had spectral lines that were red-shifted, indicating that they were moving away from the Earth, some at speeds of up to 1000?km/s. Motion at high speed is not uncommon in the cosmos—the Sun, for example, orbits around the center of our Galaxy at 240 km/s.作者: 大門在匯總 時(shí)間: 2025-3-28 11:55 作者: 現(xiàn)暈光 時(shí)間: 2025-3-28 18:17
Structure Formations are grouped in clusters, which are in turn grouped into still larger structures, called superclusters. The formation of cosmic structures is an active area of research, and we now believe we have a good idea of how they emerged.作者: BUCK 時(shí)間: 2025-3-28 21:24 作者: 協(xié)定 時(shí)間: 2025-3-29 01:16
Niamh Stephenson,Dimitris Papadopouloseriously had spectral lines that were red-shifted, indicating that they were moving away from the Earth, some at speeds of up to 1000?km/s. Motion at high speed is not uncommon in the cosmos—the Sun, for example, orbits around the center of our Galaxy at 240 km/s.作者: 使虛弱 時(shí)間: 2025-3-29 04:15
Sean F. Edgecomb,Benjamin Gillespiend that the universe was denser in its past than it is today. In fact, the density of the universe grows without bound as we wind the clock back to the big bang. Furthermore, the temperature of the universe also soars to extremely high values. How do we know this? And what does this imply about the conditions of the early universe?作者: delta-waves 時(shí)間: 2025-3-29 09:28 作者: irritation 時(shí)間: 2025-3-29 14:33 作者: 減少 時(shí)間: 2025-3-29 17:05 作者: 無能性 時(shí)間: 2025-3-29 22:14 作者: 結(jié)束 時(shí)間: 2025-3-29 23:57
https://doi.org/10.1007/978-3-319-45044-5In his monumental . Newton formulated the general laws of motion and the law of universal gravitation. He then applied these laws to explain the motion of planets and comets, projectile trajectories, and the marine tides, among other things.作者: 錫箔紙 時(shí)間: 2025-3-30 06:42 作者: hegemony 時(shí)間: 2025-3-30 09:30
Niamh Stephenson,Dimitris PapadopoulosWill the universe continue to expand forever, or will it eventually halt and start to collapse?作者: Carcinogen 時(shí)間: 2025-3-30 15:33 作者: 討好女人 時(shí)間: 2025-3-30 20:36
Karl W. W?ber,Daniel R. FesenmaierThe hot big bang cosmology that we have discussed so far has been a very successful theory作者: fixed-joint 時(shí)間: 2025-3-30 21:34 作者: surrogate 時(shí)間: 2025-3-31 00:57 作者: jettison 時(shí)間: 2025-3-31 06:38
