According to the separate universe conjecture, spherically symmetric sub-regions in an isotropic universe behave like mini-universes with their own cosmological parameters. This is an excellent approximation in both Newtonian and general relativistic theories. We estimate local expansion rates for a large number of such regions, and use a scale parameter calculated from the volume-averaged increments of local scale parameters at each time step in an otherwise standard cosmological N -body simulation. The particle mass, corresponding to a coarse graining scale, is an adjustable parameter. This mean field approximation neglects tidal forces and boundary effects, but it is the first step towards a non-perturbative statistical estimation of the effect of non-linear evolution of structure on the expansion rate. Using our algorithm, a simulation with an initial Ω m = 1 Einstein-de Sitter setting closely tracks the expansion and structure growth history of the ΛCDM cosmology. Due to small but characteristic differences, our model can be distinguished from the ΛCDM model by future precision observations. Moreover, our model can resolve the emerging tension between local Hubble constant measurements and the Planck best-fitting cosmology. Further improvements to the simulation are necessary to investigate light propagation and confirm full consistency with cosmic microwave background observations.
The recent AvERA cosmological simulation of Rácz et al. (2017) has a ΛCDMlike expansion history and removes the tension between local and Planck (cosmic microwave background) Hubble constants. We contrast the AvERA prediction of the integrated Sachs-Wolfe (ISW) effect with that of ΛCDM. The linear ISW effect is proportional to the derivative of the growth function, thus it is sensitive to small differences in the expansion histories of the respective models. We create simulated ISW maps tracing the path of light-rays through the Millennium XXL cosmological simulation, and perform theoretical calculations of the ISW power spectrum. AvERA predicts a significantly higher ISW effect than ΛCDM, A = 1.93 − 5.29 times larger depending on the l index of the spherical power spectrum, which could be utilized to definitively differentiate the models. We also show that AvERA predicts an oppositesign ISW effect in the redshift range z ≈ 1.5 − 4.4, in clear contrast with ΛCDM. Finally, we compare our ISW predictions with previous observations. While at present these cannot distinguish between the two models due to large error bars, and lack of internal consistency suggesting systematics, ISW probes from future surveys will tightly constrain the models.
Unlike NASA's original Kepler Discovery Mission, the renewed K2 Mission will stare at the plane of the Ecliptic, observing each field for approximately 75 days. This will bring new opportunities and challenges, in particular the presence of a large number of main-belt asteroids that will contaminate the photometry. The large pixel size makes K2 data susceptible to the effect of apparent minor planet encounters. Here we investigate the effects of asteroid encounters on photometric precision using a sub-sample of the K2 Engineering data taken in February, 2014. We show examples of asteroid contamination to facilitate their recognition and distinguish these events from other error sources. We conclude that main-belt asteroids will have considerable effects on K2 photometry of a large number of photometric targets during the Mission, that will have to be taken into account. These results will be readily applicable for future space photometric missions applying large-format CCDs, such as TESS and PLATO.
Hantaviruses (Bunyaviridae) cause hemorrhagic fever with renal syndrome (HFRS) in Eurasia and hantavirus (cardio)pulmonary syndrome (HCPS) in the Americas. HFRS is caused by Hantaan virus (HTNV), Seoul virus (SEOV), Dobrava virus (DOBV), Saaremaa virus (SAAV), and Puumala virus (PUUV). Of those, only HTNV is not present in Europe. In recent years, hantaviruses, described in other parts of Europe, were also detected at various locations in Hungary. To study the genetic properties of Hungarian hantaviruses in detail, sequences of the viral S and M segments were recovered from bank voles (Myodes glareolus), yellow‐necked mice (Apodemus flavicollis), and striped field mice (Apodemus agrarius) trapped in the Transdanubian region. As expected, the sequences recovered belonged, respectively, to PUUV (two strains), DOBV (one strain), and SAAV (one strain). On phylogenetic trees two new Hungarian PUUV strains located within the well‐ supported Alpe‐Adrian (ALAD) genetic lineage that included also Austrian, Slovenian, and Croatian strains. Analysis of the Hungarian SAAV and DOBV genetic variants showed host‐specific clustering and also geographical clustering within each of these hantavirus species. Hungarian SAAV and DOBV strains were related most closely to strains from Slovenia (Prekmurje region). This study confirms that multiple hantaviruses can co‐circulate in the same locality and can be maintained side‐by‐side in different rodent species. J. Med. Virol. 81:2045–2052, 2009. © 2009 Wiley‐Liss, Inc.
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