The real- and redshift-space density distribution functions for large-scale structure in the spherical collapse approximation     

Robert J. Scherrer  Enrique Gaztañaga 《Monthly notices of the Royal Astronomical Society》2001,328(1):257-265

We use the spherical collapse (SC) approximation to derive expressions for the smoothed redshift-space probability distribution function (PDF), as well as the p -order hierarchical amplitudes S _p , in both real and redshift space. We compare our results with numerical simulations, focusing on the     standard CDM model, where redshift distortions are strongest. We find good agreement between the SC predictions and the numerical PDF in real space even for     , where σ _L is the linearly evolved rms fluctuation on the smoothing scale. In redshift space, reasonable agreement is possible only for     . Numerical simulations also yield a simple empirical relation between the real-space PDF and the redshift-space PDF: we find that for     , the redshift-space PDF, [ P δ _{( z )}], is, to a good approximation, a simple rescaling of the real-space PDF, P [ δ ], i.e.,     where σ and σ _{( z )} are the real-space and redshift-space rms fluctuations, respectively. This result applies well beyond the validity of linear perturbation theory, and it is a good fit for both the standard CDM model and the ΛCDM model. It breaks down for SCDM at     , but provides a good fit to the ΛCDM models for σ _L as large as 0.8.  相似文献   

Long-Term Evolution of the Seismic Activity Preceding the 2015 Seismic Crisis at Deception Island Volcano,Antarctica (2008-2015)     

Jiménez-Morales  Vanessa  Almendros  Javier  Carmona  Enrique 《Surveys in Geophysics》2022,43(3):959-994

Surveys in Geophysics - Deception Island is an active volcano located in the South Shetland Islands, Antarctica. Although the last eruptions occurred in 1967-1970, the volcano has undergone periods...  相似文献   

Sorption and desorption behavior of residual antidepressants and caffeine in freshwater sediment and sewage sludge   总被引：1，自引：0，他引：1  

Ismael Laurindo Costa Junior  Christiane Schinneider Machado  Adelmo Lowe Pletsch  Yohandra Reyes Torres 《国际泥沙研究》2022,37(3):346-354

The use of antidepressants is widespread in modern times. Thus, they present a potential risk for ecosystems due to occurrence in domestic sewage containing unaltered metabolites and structures, even after the treatment plants have processed the sewage. The current research investigated the sorption and desorption of antidepressants(citalopram, venlafaxine, fluoxetine, sertraline, and amitriptyline) and caffeine from freshwater sediment and sewage sludge. The samples of freshwater sediment were ...  相似文献   

Cratering and modification of wet‐target craters: Projectile impact experiments and field observations of the Lockne marine‐target crater (Sweden)     

Jens Orm  Maurits Lindstrm  Alain Lepinette  Jesús Martinez‐Frias  Enrique Diaz‐Martinez 《Meteoritics & planetary science》2006,41(10):1605-1612

Abstract— Marine impacts are one category of crater formation in volatile targets. At target water depths exceeding the diameter of the impactor, the zones of vaporization, melting, and excavation of the standard land‐target cratering model develop partially or entirely in the water column. The part of the crater that has a potential of being preserved (seafloor crater) may to a great extent be formed by material emplacement and excavation processes that are very different from land‐target craters. These processes include a high‐energy, water‐jet‐driven excavation flow. At greater water depths, the difference in strength of the target layers causes a concentric crater to evolve. The crater consists of a wide water cavity with a shallow excavation flow along the seabed surrounding a nested, deeper crater in the basement. The modification of the crater is likewise influenced by the water through its forceful resurge to fill the cavity in the water mass and the seafloor. The resurge flow is strongly erosive and incorporates both ejecta and rip‐up material from the seabed surrounding the excavated crater. A combination of field observations and impact experiments has helped us analyze the processes affecting the zone between the basement crater and the maximum extent of the water cavity. The resurge erosion is facilitated by fragmentation of the upper parts of the solid target caused by a) spallation and b) vibrations from the shallow excavation flow and, subsequently, c) the vertical collapse of the water cavity rim wall. In addition, poorly consolidated and saturated sediments may collapse extensively, possibly aided by a violent expansion of the pore water volume when it turns into a spray during passage of the rarefaction wave. This process may also occur at impacts into water‐saturated targets without an upper layer of seawater present. Our results have implications for impacts on both Earth and Mars, and possibly anywhere in the solar system where volatiles exist/have existed in the upper part of the target.  相似文献   

The white dwarf luminosity function – I. Statistical errors and alternatives     

Enrique M. Geijo  Santiago Torres  Jordi Isern  Enrique García-Berro 《Monthly notices of the Royal Astronomical Society》2006,369(4):1654-1666

  相似文献   

Parametric analysis of gravity offshore structures: Part 2     

Jaime Dominguez  Enrique Alarcon 《Applied Ocean Research》1981,3(3):101-104

  相似文献   

Factors affecting wave magnitude and period during the earthquakes of September, 1985     

Enrique del Valle Toledo 《Geotechnical and Geological Engineering》1989,7(1):29-35

Summary The geology and structure of the Mexico Basin are discussed and hypotheses developed to explain the magnification of wave amplitudes during the 1985 earthquake.  相似文献   

Preface     

Enrique Pérez  Richard de Grijs  Rosa M. González Delgado 《Astrophysics and Space Science》2009,324(2-4):79-81

  相似文献   

Rebuttal to “Comment on “Evidence of electrical activity on Titan drawn from the Schumann resonances sent by Huygens probe” by J.A. Morente, J.A. Portí, A. Salinas, and E.A. Navarro [2008, Icarus, 195, 802-811]”     

Juan A. Morente  Jorge A. Portí  Enrique A. Navarro 《Icarus》2009,204(1):352-354

Hamelin et al. criticize some conclusions of our paper [Morente, J.A., Portí, J.A., Salinas, A., Navarro, E.A., 2008. Icarus 195, 802-811]. This rebuttal is our response to their criticism. In our view, their comments are contradictory and not based on scientific argument. Our paper presents a comprehensible methodology for extracting weak resonances from the late-time response of systems with high losses and our conclusions are derived from and supported by this methodology, which was first checked using an analytical function and later with the data from a numerical simulation of Titan’s atmosphere. Conversely, the Comment of Hamelin et al. does not contain any mathematical proof, either supporting their statements or invalidating our analysis procedure.  相似文献   

Stable isotope and fluid inclusion data of the Rooiberg tin field deposits,South Africa     

Kevin Faure  Agnes Reyes 《Journal of Geochemical Exploration》2009

  相似文献