標(biāo)題: Titlebook: Generation of Cosmological Large-Scale Structure; David N. Schramm,P. Galeotti Book 1997 Kluwer Academic Publishers 1997 Astronomical Obse [打印本頁] 作者: 不友善 時間: 2025-3-21 20:09
書目名稱Generation of Cosmological Large-Scale Structure影響因子(影響力)
書目名稱Generation of Cosmological Large-Scale Structure影響因子(影響力)學(xué)科排名
書目名稱Generation of Cosmological Large-Scale Structure網(wǎng)絡(luò)公開度
書目名稱Generation of Cosmological Large-Scale Structure網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Generation of Cosmological Large-Scale Structure被引頻次
書目名稱Generation of Cosmological Large-Scale Structure被引頻次學(xué)科排名
書目名稱Generation of Cosmological Large-Scale Structure年度引用
書目名稱Generation of Cosmological Large-Scale Structure年度引用學(xué)科排名
書目名稱Generation of Cosmological Large-Scale Structure讀者反饋
書目名稱Generation of Cosmological Large-Scale Structure讀者反饋學(xué)科排名
作者: 人類學(xué)家 時間: 2025-3-21 21:51
https://doi.org/10.1007/978-1-4419-6330-7 more complex than two-point statistics, primarily because of the combinatorial explosion of terms and the large number of parameters involved. For this reason special techniques are necessary for the extraction of cosmologically important information.作者: 運(yùn)動的我 時間: 2025-3-22 01:06
https://doi.org/10.1007/978-4-431-55040-2utions as one of three topological types: connected, structureless or clumpy. Connected topologies are consistent with galaxy distributions described as filaments or sheets. Clumpy topologies are often referred to as “meatball” topologies where aggregates of galaxies are surrounded and separated by voids.作者: Euphonious 時間: 2025-3-22 05:43 作者: Induction 時間: 2025-3-22 11:48 作者: FEAS 時間: 2025-3-22 15:05
DARK MATTER: An Introductionons as well as the other light element abundancea are examined in detail. Comparison of nucleosynthesis baryonic density arguments with other baryon density arguments is made. Discussion of the interface of density and age arguments is also presented.作者: FEAS 時間: 2025-3-22 20:58 作者: 枯燥 時間: 2025-3-22 23:37
A Two-Dimensional Percolation Analysis of the Las Campanas Redshift Surveyutions as one of three topological types: connected, structureless or clumpy. Connected topologies are consistent with galaxy distributions described as filaments or sheets. Clumpy topologies are often referred to as “meatball” topologies where aggregates of galaxies are surrounded and separated by voids.作者: objection 時間: 2025-3-23 04:35 作者: 愛管閑事 時間: 2025-3-23 09:16
The Findings: Dependent Variables,surements of both the absolute temperature and the anisotropy of the CMB and discuss the relation between the data and the general theoretical framework. Future directions are indicated and the upcoming satellite experiments are discussed.作者: 嘴唇可修剪 時間: 2025-3-23 13:15
https://doi.org/10.1007/978-3-662-64682-3es which are insensitive to large scale structure require that only the normalization, not the shape, of the luminosity function vary with radial position. In the final two sections of this chapter we will see that this is not strictly true.作者: 租約 時間: 2025-3-23 15:59
Methodologies, Methods and Data,getic and less accurately predicted .B-neutrinos, is in the range of predicted values. That means, depending on the underlying SSM, there is a deficit of neutrinos or not. Combining the Kamiokande result with the data of the radiochemical Homestake-experiment [5] the derived flux for the .Be-neutrinos seems to be strongly suppressed for all SSM’s.作者: musicologist 時間: 2025-3-23 21:51
Conversations Around Semiotic Engineering in terms of number of structures and sphericity for different values of the threshold detection and at all the scales investigated. According to our analysis, there is strong evidence for multiple hierarchical substructure, on the scales ranging from a few hundreds of Kpc to about 4.. Mpc, and the substructure morphology is rather spherical.作者: 婚姻生活 時間: 2025-3-23 22:57
Conversations in Postcolonial Thoughtxy counts ... In Section 2 we give a brief description of the way we use Minkowski functionals, in Section 3 we present the results for the Minkowski functionals obtained from the IRAS 1.2 Jy galaxy catalogue (the results for next—neighbour distributions and .. will be present in Kerscher et al. [6]), and in Section 4 we discuss our results.作者: colony 時間: 2025-3-24 03:00
High Redshift Galaxiesellent to understand some of the details of the grand design of Nature. A variety of unforeseen facts are being, and expect to be, discovered. The advent of advanced detector technology, fast computer facilities and large telescopes are making all of this possible.作者: Volatile-Oils 時間: 2025-3-24 10:15
On Observing the Cosmic Microwave Backgroundsurements of both the absolute temperature and the anisotropy of the CMB and discuss the relation between the data and the general theoretical framework. Future directions are indicated and the upcoming satellite experiments are discussed.作者: Employee 時間: 2025-3-24 11:48 作者: inferno 時間: 2025-3-24 16:02 作者: 嬉耍 時間: 2025-3-24 21:52 作者: SPECT 時間: 2025-3-24 23:46
Fluctuations in the IRAS 1.2 Jy Cataloguexy counts ... In Section 2 we give a brief description of the way we use Minkowski functionals, in Section 3 we present the results for the Minkowski functionals obtained from the IRAS 1.2 Jy galaxy catalogue (the results for next—neighbour distributions and .. will be present in Kerscher et al. [6]), and in Section 4 we discuss our results.作者: gerontocracy 時間: 2025-3-25 03:36 作者: CRAB 時間: 2025-3-25 10:49 作者: 暴露他抗議 時間: 2025-3-25 15:13 作者: esculent 時間: 2025-3-25 16:47 作者: QUAIL 時間: 2025-3-25 22:45 作者: pericardium 時間: 2025-3-26 02:38
the current situation on the age of the universe and the Hubble constant are reviewed since they provide the framework for the basic density arguments. It is shown that the Big Bang Nucleosynthesis constraints on the cosmological baryon density, when compared with dynamical arguments, demonstrate th作者: Prostatism 時間: 2025-3-26 07:10
https://doi.org/10.1007/978-94-009-8024-2er distribution. The amplitude of those velocities is regulated by the spatial scale and the amplitude of the matter density irregularities as well as by the value of the mean matter density. The direct measurement of peculiar velocities thus provides a means to infer the characteristics of the mass作者: exophthalmos 時間: 2025-3-26 11:46 作者: 凹室 時間: 2025-3-26 16:33
https://doi.org/10.1007/978-3-662-64682-3luminosity. In this chapter I review some topics which I considered in my thesis. In the presence of large scale structure sophisticated techniques are needed for luminosity function. I will discuss one of these and its extension to a photometric data set. All luminosity function estimation techniqu作者: Ankylo- 時間: 2025-3-26 18:37
Methodologies, Methods and Data,on the range of predictions of several Standard Solar Models (SSM) [1] [2] [3] is listed for each type of experiment together with the calculated contributions of the strongest solar neutrino branches. A basic analysis shows that the result of Kamiokande [4], which is only sensitive to the high ener作者: Condescending 時間: 2025-3-26 22:36 作者: Dysarthria 時間: 2025-3-27 02:16
Conversations Around Semiotic Engineeringtructure analysis method is based on the wavelet transform and on the segmentation analysis. The wavelet transform allows us to find out structures at different scales and the segmentation method allows us a quantitative statistical and morphological analysis of the sample. Our results are expressed作者: 彎彎曲曲 時間: 2025-3-27 06:02
Conversations in Postcolonial Thoughts), we found that the clustering properties of galaxies differ significantly in the northern and southern parts, showing fluctuations in the clustering properties at least on scales of 200..Mpc. Our analysis is based on Minkowski functionals, next—neighbour distributions, and the fluctuation of gala作者: 滋養(yǎng) 時間: 2025-3-27 13:05 作者: Munificent 時間: 2025-3-27 14:40 作者: byline 時間: 2025-3-27 21:36
Generation of Cosmological Large-Scale Structure978-94-009-0053-0Series ISSN 1389-2185 作者: HEDGE 時間: 2025-3-28 00:31
Olivier de Bandt,Jean-Pierre Villetellehe other hand, the universe is extremely clumpy on small scales . ≤ 1.. The inhomogeneities in the intermediate range of scales — groups and clusters of galaxies, superclusters and voids — that are collectively termed as the large scale structure of the universe (hereafter LSS) show a variety of shapes and sizes.作者: 不能強(qiáng)迫我 時間: 2025-3-28 04:57
https://doi.org/10.1007/978-3-031-36163-0r other observed tracers of cosmic structure, including both normal and active galaxies. Mounting evidence that the high column density absorbers are young galaxies links relatively pristine baryonic matter to highly evolved objects at the present day ([1-3] and references therein).作者: GRE 時間: 2025-3-28 08:45
Dynamics of the Large-Scale Structurehe other hand, the universe is extremely clumpy on small scales . ≤ 1.. The inhomogeneities in the intermediate range of scales — groups and clusters of galaxies, superclusters and voids — that are collectively termed as the large scale structure of the universe (hereafter LSS) show a variety of shapes and sizes.作者: Exposition 時間: 2025-3-28 11:18 作者: Enliven 時間: 2025-3-28 15:39
https://doi.org/10.1007/978-94-009-0053-0Astronomical Observation; Cosmology; Dark matter; Redshift; Universe; astronomy; astrophysics作者: 事物的方面 時間: 2025-3-28 19:58 作者: Expand 時間: 2025-3-29 01:17
https://doi.org/10.1007/978-3-031-19127-5Dynamical and redshift distortion studies can give Ω. only in the combination . = Ω./.. The determination of the density parameter Ω. by such methods is therefore impossible without a measurement of the bias parameter ..作者: GRAIN 時間: 2025-3-29 05:56
Harmonizing the Babel of VoicesEver since the first high-quality galaxy catalogues became available, statistics of large-scale structure has been an important tool to gain insight into the underlying physical processes and to allow for comparison of observations and predictions, both through theory and numerical experiment.作者: 前奏曲 時間: 2025-3-29 08:39
Conversations on Optimal TransportWe study the evolution of the mass autocorrelation function in the Zel’dovich approximation and we compare the results with the predictions of the scaling ansatz for the growth of gravitational clustering formulated by Jain, Mo & White [7].作者: 助記 時間: 2025-3-29 11:28
On the Cosmological Mass FunctionThe theoretical determination of the mass function is performed by means of Lagrangian perturbation theory and ellipsoidal collapse. The statistical framework necessary to determine the mass function is briefly described. The main results and future applications are outlined.作者: 帶來 時間: 2025-3-29 15:52 作者: 窗簾等 時間: 2025-3-29 22:25 作者: legislate 時間: 2025-3-30 02:00 作者: 黑豹 時間: 2025-3-30 06:29
High Redshift Galaxiesexcitement in current cosmology, as mentioned also by J. Peebles sometime before 1983, is that we have opened an observational and theoretical window in the world of mathematical models and we are now looking in them, confronting them with the observations with the feeling that the prospects are exc作者: 煩人 時間: 2025-3-30 10:05 作者: 連累 時間: 2025-3-30 15:45 作者: reflection 時間: 2025-3-30 18:57 作者: Priapism 時間: 2025-3-30 21:13 作者: 繁殖 時間: 2025-3-31 01:24
DARK MATTER: An Introductionthe current situation on the age of the universe and the Hubble constant are reviewed since they provide the framework for the basic density arguments. It is shown that the Big Bang Nucleosynthesis constraints on the cosmological baryon density, when compared with dynamical arguments, demonstrate th作者: 走調(diào) 時間: 2025-3-31 07:01 作者: 忙碌 時間: 2025-3-31 13:13 作者: 依法逮捕 時間: 2025-3-31 15:12 作者: Orthodontics 時間: 2025-3-31 19:26
Spectroscopy of Solar Neutrinos with Borexinoon the range of predictions of several Standard Solar Models (SSM) [1] [2] [3] is listed for each type of experiment together with the calculated contributions of the strongest solar neutrino branches. A basic analysis shows that the result of Kamiokande [4], which is only sensitive to the high ener作者: PON 時間: 2025-4-1 00:39
A Two-Dimensional Percolation Analysis of the Las Campanas Redshift Surveyucture in a galaxy distribution and characterizing the topology of a distribution that is not random noise. Percolation analysis characterizes distributions as one of three topological types: connected, structureless or clumpy. Connected topologies are consistent with galaxy distributions described 作者: confederacy 時間: 2025-4-1 02:59
A Wavelet Analysis of the Coma Clustertructure analysis method is based on the wavelet transform and on the segmentation analysis. The wavelet transform allows us to find out structures at different scales and the segmentation method allows us a quantitative statistical and morphological analysis of the sample. Our results are expressed
