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標(biāo)題: Titlebook: Cosmological Pattern of Microphysics in the Inflationary Universe; Maxim Yu. Khlopov,Sergei G. Rubin Book 2004 Springer Science+Business M [打印本頁]

作者: HAVEN    時間: 2025-3-21 20:03
書目名稱Cosmological Pattern of Microphysics in the Inflationary Universe影響因子(影響力)




書目名稱Cosmological Pattern of Microphysics in the Inflationary Universe影響因子(影響力)學(xué)科排名




書目名稱Cosmological Pattern of Microphysics in the Inflationary Universe網(wǎng)絡(luò)公開度




書目名稱Cosmological Pattern of Microphysics in the Inflationary Universe網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱Cosmological Pattern of Microphysics in the Inflationary Universe被引頻次




書目名稱Cosmological Pattern of Microphysics in the Inflationary Universe被引頻次學(xué)科排名




書目名稱Cosmological Pattern of Microphysics in the Inflationary Universe年度引用




書目名稱Cosmological Pattern of Microphysics in the Inflationary Universe年度引用學(xué)科排名




書目名稱Cosmological Pattern of Microphysics in the Inflationary Universe讀者反饋




書目名稱Cosmological Pattern of Microphysics in the Inflationary Universe讀者反饋學(xué)科排名





作者: BRACE    時間: 2025-3-21 23:50

作者: FRET    時間: 2025-3-22 01:43
Cosmological Pattern of Microphysics in the Inflationary Universe
作者: 感情脆弱    時間: 2025-3-22 07:25

作者: 不舒服    時間: 2025-3-22 11:55

作者: 分解    時間: 2025-3-22 15:49
https://doi.org/10.1007/978-3-322-80645-1the hidden sector of particle theory. Such particles, fields and mechanisms may play an important role in the problem of UHECR. It makes new physics a necessary component of the analysis of UHECR data.
作者: 分解    時間: 2025-3-22 18:47
0168-1222 obes for these ideas, linking their predictions to their possible experimental test. We use the framework of in?ationary paradigm to reveal the phenomena that can shed light on the physical origin of the observ978-90-481-6695-4978-1-4020-2650-8Series ISSN 0168-1222 Series E-ISSN 2365-6425
作者: MAOIS    時間: 2025-3-22 23:03

作者: 催眠藥    時間: 2025-3-23 03:46
Fine-Tuning of Microphysical Parameters in the Universe,t is worth mentioning the existence of dark matter and dark energy, of superhigh energy particles in cosmic rays and ‘bursts’ an almost instantaneous energy explosion with energy release of order l0. erg. These astrophysical data specify presence of the new phenomena, which should be comprehended.
作者: 泄露    時間: 2025-3-23 05:42

作者: 拱墻    時間: 2025-3-23 09:49
0168-1222 g the interactions between different cosmological phenomena Modern cosmology is a quickly developing ?eld of research. New technical devices and tools supply the community with new experimental data measured with high accuracy. The self-consistent explanation of these data needs t- oretical models t
作者: ICLE    時間: 2025-3-23 14:48
,Der Sozialversicherungsstaat in N?ten,um state. Energy is perfectly localized, and density is slightly pulsating around its maximum. This process is accompanied by radiation of scalar waves. Under some conditions the localization of enemy leads to formation of small black holes with high probability.
作者: output    時間: 2025-3-23 20:11
Fazit: Variationen des konservativen Typs,t is worth mentioning the existence of dark matter and dark energy, of superhigh energy particles in cosmic rays and ‘bursts’ an almost instantaneous energy explosion with energy release of order l0. erg. These astrophysical data specify presence of the new phenomena, which should be comprehended.
作者: 幻影    時間: 2025-3-23 22:24
,Der Sozialversicherungsstaat in N?ten, near future. Such searches involve both direct search for pieces of antimatter — for antinuclei or antimeteorites, or use indirect probes by gamma radiation that may be originated from antimatter annihilation.
作者: magenta    時間: 2025-3-24 05:27
Antimatter in the Modern Universe, near future. Such searches involve both direct search for pieces of antimatter — for antinuclei or antimeteorites, or use indirect probes by gamma radiation that may be originated from antimatter annihilation.
作者: 柳樹;枯黃    時間: 2025-3-24 09:32

作者: 畫布    時間: 2025-3-24 13:08

作者: 構(gòu)想    時間: 2025-3-24 17:23

作者: analogous    時間: 2025-3-24 20:56
Basis of Inflation,erproduction of the inflationary models, a number of which increase constantly. Below we discuss the properties of inflationary scenario on the basis of chaotic inflation. Some other models are considered in Chapter 10 to give imagination on the beauty and rich possibilities of the inflationary paradigm.
作者: 傳授知識    時間: 2025-3-25 02:02
Nationen als Gerechtigkeitskooperativrically, it reminds us of the links between statistical physics and thermodynamics, or between electrodynamics and theory of electron. To the end of the XX Century a new level of this relationship was realized, linking the science of the Universe as a whole and physics of elementary particles.
作者: Perennial長期的    時間: 2025-3-25 04:49

作者: nonplus    時間: 2025-3-25 07:30

作者: Stricture    時間: 2025-3-25 12:15

作者: jumble    時間: 2025-3-25 17:41

作者: 豐富    時間: 2025-3-25 21:41

作者: CAB    時間: 2025-3-26 02:52
https://doi.org/10.1007/978-3-322-80645-1e physics and cosmology in the analysis of their possible origin and effects. Even for known particles and interactions UHECR correspond to the energy range at which their properties were not studied experimentally. Particle theory predicts a wide variety of new phenomena in this energy range. One s
作者: cancer    時間: 2025-3-26 04:59

作者: 效果    時間: 2025-3-26 09:40
Fazit: Variationen des konservativen Typs,ch we expected to be discovered for a long time, are still only hypotheses. Other data, being very impressive, are yet not explained. As an example, it is worth mentioning the existence of dark matter and dark energy, of superhigh energy particles in cosmic rays and ‘bursts’ an almost instantaneous
作者: Regurgitation    時間: 2025-3-26 14:48

作者: PON    時間: 2025-3-26 19:00

作者: 國家明智    時間: 2025-3-26 21:57
978-90-481-6695-4Springer Science+Business Media Dordrecht 2004
作者: dialect    時間: 2025-3-27 01:10

作者: chondromalacia    時間: 2025-3-27 07:33
Strong Primordial Inhomogeneities and Galaxy Formation,rav-itational instability from small initial perturbations of density or gravitational potential. As a rule, these perturbations are Gaussian, but some versions of non-Gaussian perturbations are also discussed.
作者: 合乎習(xí)俗    時間: 2025-3-27 11:49

作者: DRAFT    時間: 2025-3-27 16:38
Maxim Yu. Khlopov,Sergei G. RubinAn introduction into the inflationary scenario of, and the crucial role of quantum fluctuations in the evolution of the Universe - clarifying the interactions between different cosmological phenomena
作者: 容易懂得    時間: 2025-3-27 18:28
Fundamental Theories of Physicshttp://image.papertrans.cn/c/image/238920.jpg
作者: 觀點    時間: 2025-3-28 01:26
Cosmological Pattern of Microphysics in the Inflationary Universe978-1-4020-2650-8Series ISSN 0168-1222 Series E-ISSN 2365-6425
作者: 迅速成長    時間: 2025-3-28 02:14

作者: 言外之意    時間: 2025-3-28 06:47

作者: Tremor    時間: 2025-3-28 12:52
https://doi.org/10.1007/978-3-322-80645-1 a very interesting and important period of the evolution of our Universe. A lot of observational data can find new nontrivial explanation in this framework. In addition, new phenomena are predicted, some of them having been discussed in this book.
作者: Comedienne    時間: 2025-3-28 16:43
Welche Zukunft für den Sozialstaat?As a result, we realize that there are a large number of inflationary models elaborated up to now. Some of them are purely phenomenological, others have some theoretical basis. The main problem now is to choose one that describes observational data, which became much richer and refined during the last decade.
作者: 金桌活畫面    時間: 2025-3-28 19:04

作者: 落葉劑    時間: 2025-3-29 01:38

作者: Inscrutable    時間: 2025-3-29 04:05
Basis of Inflation,he explanation of the observable Universe was so impressive that the majority of scientists had no doubts on its correctness, at least as the basic principle, Unfortunately (or maybe, on the contrary, fortunately) the mechanism of inflation may be put into practice by a variety of ways. It led to ov
作者: intention    時間: 2025-3-29 08:44

作者: Frisky    時間: 2025-3-29 13:15
Strong Primordial Inhomogeneities and Galaxy Formation,rav-itational instability from small initial perturbations of density or gravitational potential. As a rule, these perturbations are Gaussian, but some versions of non-Gaussian perturbations are also discussed.
作者: 萬靈丹    時間: 2025-3-29 17:38

作者: milligram    時間: 2025-3-29 21:09

作者: Clumsy    時間: 2025-3-30 02:21

作者: 機械    時間: 2025-3-30 07:14

作者: padding    時間: 2025-3-30 11:12
Fine-Tuning of Microphysical Parameters in the Universe,ch we expected to be discovered for a long time, are still only hypotheses. Other data, being very impressive, are yet not explained. As an example, it is worth mentioning the existence of dark matter and dark energy, of superhigh energy particles in cosmic rays and ‘bursts’ an almost instantaneous
作者: RAG    時間: 2025-3-30 12:23

作者: Obvious    時間: 2025-3-30 17:51





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