標(biāo)題: Titlebook: Current Topics in Astrofundamental Physics: The Cosmic Microwave Background; Norma G. Sánchez Book 2001 Kluwer Academic Publishers 2001 Ac [打印本頁] 作者: Madison 時(shí)間: 2025-3-21 18:56
書目名稱Current Topics in Astrofundamental Physics: The Cosmic Microwave Background影響因子(影響力)
書目名稱Current Topics in Astrofundamental Physics: The Cosmic Microwave Background影響因子(影響力)學(xué)科排名
書目名稱Current Topics in Astrofundamental Physics: The Cosmic Microwave Background網(wǎng)絡(luò)公開度
書目名稱Current Topics in Astrofundamental Physics: The Cosmic Microwave Background網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Current Topics in Astrofundamental Physics: The Cosmic Microwave Background被引頻次
書目名稱Current Topics in Astrofundamental Physics: The Cosmic Microwave Background被引頻次學(xué)科排名
書目名稱Current Topics in Astrofundamental Physics: The Cosmic Microwave Background年度引用
書目名稱Current Topics in Astrofundamental Physics: The Cosmic Microwave Background年度引用學(xué)科排名
書目名稱Current Topics in Astrofundamental Physics: The Cosmic Microwave Background讀者反饋
書目名稱Current Topics in Astrofundamental Physics: The Cosmic Microwave Background讀者反饋學(xué)科排名
作者: originality 時(shí)間: 2025-3-21 22:10 作者: 勾引 時(shí)間: 2025-3-22 01:40 作者: concentrate 時(shí)間: 2025-3-22 04:46
https://doi.org/10.1007/978-3-319-17428-0tructure of the polarization field would be effective for further investigation of the primordial signal and noise in the maps of anisotropy and polarization of the cosmic microwave background. Also we discuss the classification of singular points of the vector field of the CMB polarization where po作者: insipid 時(shí)間: 2025-3-22 11:51 作者: 不適當(dāng) 時(shí)間: 2025-3-22 15:42 作者: 不適當(dāng) 時(shí)間: 2025-3-22 19:07
S. Valero,E. del Val,J. Alemany,V. Bottiity predicted by CDM. The core radius .. and halo circular velocity .. are related by ..=0.44(..).., analogous to the scaling of degenerate dwarf stars. Particle velocities also filter primordial perturbations, with a filtering scale κ. ∝ ..Ω.(.ρ.).. Particle candidates for warm matter are briefly d作者: thalamus 時(shí)間: 2025-3-22 23:36 作者: Implicit 時(shí)間: 2025-3-23 04:08
Minimal String Driven Cosmology and its Predictionsr order corrections and graceful exit of inflation, we find this model closer to the observational Universe properties than the current available string cosmology scenarii. At a more fundamental level, this model is by its construction close to the standard cosmological evolution, and it is driven s作者: 模仿 時(shí)間: 2025-3-23 09:20
Some problems of the CMB polarizationtructure of the polarization field would be effective for further investigation of the primordial signal and noise in the maps of anisotropy and polarization of the cosmic microwave background. Also we discuss the classification of singular points of the vector field of the CMB polarization where po作者: Measured 時(shí)間: 2025-3-23 11:59
The High Redshift Radio Universeoch..It is shown, that Russian new generation CMBA“Cosmological Gene” project can help in the extention of the observable part of the Universe, and some questions, connected with post-SKA instrumentation will be discussed as well.作者: Notify 時(shí)間: 2025-3-23 17:48 作者: Cytology 時(shí)間: 2025-3-23 22:01 作者: corpus-callosum 時(shí)間: 2025-3-23 22:53
1389-2185 ysics framework, werethe maingoals ofthe course. Lectures ranged from a motivation and pedagogical introduction for students and participants not directly worki978-0-7923-6856-4978-94-010-0748-1Series ISSN 1389-2185 作者: 柳樹；枯黃 時(shí)間: 2025-3-24 05:23
Current Topics in Astrofundamental Physics: The Cosmic Microwave Background作者: 陶器 時(shí)間: 2025-3-24 09:37 作者: pericardium 時(shí)間: 2025-3-24 14:31 作者: Munificent 時(shí)間: 2025-3-24 17:27
New Dual Relations Between Quantum Field Theory and String Regimes In Curved BackgroundsThis operation maps the characteristic length of one regime into the other (and, as a consequence, mass domains as well). The .-transform is not an assumed or . imposed symmetry but is revealed by the QFT and String dynamics in curved backgrounds. The Hawking-Gibbons temperature and the string maxim作者: cleaver 時(shí)間: 2025-3-24 22:15
Detectability of Relic Squeezed Gravitational Waves by Laser Interferometersons, is within the reach of sensitive gravity-wave detectors. In the favorable case, the detection of relic gravitational waves can be achieved by initial laser interferometers in LIGO, VIRGO, GE0600. In more conservative cases, the sensitivity of advanced ground-based and cosmic laser interferomete作者: Conflict 時(shí)間: 2025-3-25 02:55
Gravitational Field and Its Energy-Momentum Tensorm tensor which is 1) derivable from the Lagrangian in a regular prescribed way, 2) tensor under arbitrary coordinate transformations, 3) symmetric in its components, 4) conserved due to the equations of motionderived from the same Lagrangian, 5) free of the second (highest) derivatives of the field 作者: 軟弱 時(shí)間: 2025-3-25 05:36 作者: Fracture 時(shí)間: 2025-3-25 08:50
The 1+3 Covariant Approach to CMB Anisotropiese - independent nonlinear equations for the Boltzmann radiation multipole hierarchy and linearise them about a Friedmann-Robertson-Walker model. Particular emphasis is given to the .. or . integration of the Boltzmann equation and how it compares to the usual time-like integrations presented in much作者: 職業(yè)拳擊手 時(shí)間: 2025-3-25 13:24 作者: 胰島素 時(shí)間: 2025-3-25 15:48 作者: 進(jìn)取心 時(shí)間: 2025-3-25 22:23 作者: 滑動(dòng) 時(shí)間: 2025-3-26 02:54 作者: 我怕被刺穿 時(shí)間: 2025-3-26 05:36
Clusters of Galaxies and The Large Scale Structureide angle, good space resolution and reasonably deep surveys in the X-rays. The aim of these surveys would be to observe and measure the cosmic evolution of clusters and compile a catalogue for future detailed observations using large space and ground based telescopes. We also show that the Luminosi作者: 熒光 時(shí)間: 2025-3-26 11:48 作者: 爭吵加 時(shí)間: 2025-3-26 14:43 作者: Exaggerate 時(shí)間: 2025-3-26 20:42 作者: Nonflammable 時(shí)間: 2025-3-27 00:27
Krzysztof Górecki,Ewa Krac,Janusz Zar?bskiblished observational information, we prove that it gives realistic predictions on early and current energy density and its results are compatible with General Relativity. Interestingly enough, the predicted current energy density is found Ω=1 and in any case with lower limit Ω≥4/9. On the other han作者: TERRA 時(shí)間: 2025-3-27 02:34 作者: 疏遠(yuǎn)天際 時(shí)間: 2025-3-27 07:35 作者: 概觀 時(shí)間: 2025-3-27 11:51
https://doi.org/10.1007/978-3-319-16901-9m tensor which is 1) derivable from the Lagrangian in a regular prescribed way, 2) tensor under arbitrary coordinate transformations, 3) symmetric in its components, 4) conserved due to the equations of motionderived from the same Lagrangian, 5) free of the second (highest) derivatives of the field 作者: 生氣地 時(shí)間: 2025-3-27 17:01
Springer Proceedings in Physicsin standard cosmological models.This is followed by a brief discussion of experimental techniques and contaminants, and then some recent experiments which are starting to provide the first accurate measures of the power spectrum are discussed in detail. The implications for cosmological models are d作者: 盲信者 時(shí)間: 2025-3-27 19:41 作者: 證實(shí) 時(shí)間: 2025-3-27 22:47 作者: 異教徒 時(shí)間: 2025-3-28 05:01 作者: NEX 時(shí)間: 2025-3-28 10:20 作者: BROOK 時(shí)間: 2025-3-28 13:37 作者: 聯(lián)想記憶 時(shí)間: 2025-3-28 15:26 作者: 結(jié)構(gòu) 時(shí)間: 2025-3-28 22:22
S. Valero,E. del Val,J. Alemany,V. Bottiunderstand the cosmic structure formation in the pre-virialized phase, or quasilinear règime. The emphasis is on the dynamical scaling of the multiresolution coarse-grained mass fields, which are traced by the multiscale identified clusters.作者: 叢林 時(shí)間: 2025-3-29 01:48 作者: moratorium 時(shí)間: 2025-3-29 05:42
https://doi.org/10.1007/978-94-010-0748-1Accretion; Cosmology; Dark matter; EFE; Gravity; Redshift; Renormalization group; Universe; astronomy; astrop作者: 博識 時(shí)間: 2025-3-29 09:47
978-0-7923-6856-4Kluwer Academic Publishers 2001作者: Bravado 時(shí)間: 2025-3-29 13:21 作者: BROW 時(shí)間: 2025-3-29 16:50
Structure Formation of Galaxy Clusters and Beyondunderstand the cosmic structure formation in the pre-virialized phase, or quasilinear règime. The emphasis is on the dynamical scaling of the multiresolution coarse-grained mass fields, which are traced by the multiscale identified clusters.作者: 平息 時(shí)間: 2025-3-29 22:00
Current Topics in Astrofundamental Physics: The Cosmic Microwave Background978-94-010-0748-1Series ISSN 1389-2185 作者: HALO 時(shí)間: 2025-3-30 00:43
S. Valero,E. del Val,J. Alemany,V. Bottiunderstand the cosmic structure formation in the pre-virialized phase, or quasilinear règime. The emphasis is on the dynamical scaling of the multiresolution coarse-grained mass fields, which are traced by the multiscale identified clusters.作者: CHURL 時(shí)間: 2025-3-30 07:53
29th International Symposiumon Shock Waves 2There are many familiar situations when the properties of some substance change abruptly with temperature .. For example, a liquid may be converted into a vapor or into a solid state. Phase transitions are associated with non-analyticities of the partition function of the system.作者: 前兆 時(shí)間: 2025-3-30 09:58
W. Mostert,V. Wheatley,R. SamtaneyBasic ingredients of the theory of baryogenesis are reviewed with emphasis on out-of-equilibrium decays of heavy particles. The present use of kinetic theory is explained and some attempts to go beyond the classical Boltzmann equations are discussed.作者: 好色 時(shí)間: 2025-3-30 15:49 作者: 領(lǐng)袖氣質(zhì) 時(shí)間: 2025-3-30 19:52 作者: abracadabra 時(shí)間: 2025-3-30 22:21
Book 2001 in the early universe, cosmic microwave background radiation, large scale structure, dark matter problem, and the interplay between them. The focus was placed on the Cosmic Microwave Background Radiation. Emphasis was given to the mutual impact of fundamental physics and cosmology, both at theoreti作者: 大氣層 時(shí)間: 2025-3-31 03:17 作者: engrossed 時(shí)間: 2025-3-31 05:25
David álvarez,Ramón Fernández,Lidia Sánchezall, highly dusty and involved in massive star-formation activity. Young galaxies in nearby space have been identified with HST data, but reliable ages are still very difficult to obtain. A certain rather large population of uncondensed, starless galaxies has been tentatively identified in the Local Group.作者: Flustered 時(shí)間: 2025-3-31 11:47
New Dual Relations Between Quantum Field Theory and String Regimes In Curved Backgroundsal or critical temperature are .-mapped one into the other. If hack reaction of quantum matter is included, Quantum Field Theory and String phases appear, and .-relations between them manifest as well. T hese .-transformations are explicitly shown in two relevant examples: Black Hole and de Sit ter space times.作者: 劇毒 時(shí)間: 2025-3-31 14:11
Detectability of Relic Squeezed Gravitational Waves by Laser Interferometersrs will be needed. The specific statistical signature of relic gravitational waves, associated with the phenomenon of squeezing, is a potential reserve for further improvement of the signal to noise ratio.作者: FRAUD 時(shí)間: 2025-3-31 20:33
Gravitational Field and Its Energy-Momentum Tensorvariables, and 6) is unique up to trivial modifications not containing the field variables. There is nothing else in addition to these six conditions that onecoulddemand from the energy-momentum tensor fully acceptableon physical and mathematical ground. This contribution is basedon the work [.].
