2015/08/27

X線鉄輝線共鳴散乱を用いた銀河団内高温プラズマでの乱流の大きさの制限

http://www-heaf.hepl.hiroshima-u.ac.jp/gakkai.html

枝廣育実(広島大学)

http://www.asj.or.jp/nenkai/2014b/T.html


発展し続ける一般相対論―時空論の起承転"望"―

http://www.jps.or.jp/books/gakkaishi/2015/02/702.php

一般相対論の成立 岡村 浩 ...... 81
一般相対論ミニマム 須藤 靖 ...... 87
一般相対性理論の数理 小玉英雄 ...... 95
中性子星とブラックホール―相対論的天体物理学入門― 中村卓史 ...... 103
一般相対論的宇宙論 杉山 直 ...... 111
一般相対論の実験的検証と重力理論の拡張 田中貴浩 ...... 119
アインシュタインからの宿題:重力波の検出 川村静児 ...... 125
一般相対論と量子力学の統合に向けて 大栗博司 ...... 130
数値相対論の展開 柴田 大 ...... 134

2015/08/20

Wide-field lensing mass maps from Dark Energy Survey science verification data: Methodology and detailed analysis

http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1504.03002

http://www.nature.com/news/dark-matter-mapped-at-cosmic-scale-1.17311

Weak gravitational lensing allows one to reconstruct the spatial distribution of the projected mass density across the sky. These "mass maps" provide a powerful tool for studying cosmology as they probe both luminous and dark matter. In this paper, we present a weak lensing mass map reconstructed from shear measurements in a 139 deg2 area from the Dark Energy Survey (DES) science verification data. We compare the distribution of mass with that of the foreground distribution of galaxies and clusters. The overdensities in the reconstructed map correlate well with the distribution of optically detected clusters. We demonstrate that candidate superclusters and voids along the line of sight can be identified, exploiting the tight scatter of the cluster photometric redshifts. We cross-correlate the mass map with a foreground magnitude-limited galaxy sample from the same data. Our measurement gives results consistent with mock catalogs from N -body simulations that include the primary sources of statistical uncertainties in the galaxy, lensing, and photo-z catalogs. The statistical significance of the cross-correlation is at the 6.8 σ level with 20 arcminute smoothing. We find that the contribution of systematics to the lensing mass maps is generally within measurement uncertainties. In this work, we analyze less than 3% of the final area that will be mapped by the DES; the tools and analysis techniques developed in this paper can be applied to forthcoming larger data sets from the survey.


2015/06/10

The dark side of cosmology: Dark matter and dark energy

2015-06-10
A nice review.

http://www.sciencemag.org/content/347/6226/1100.abstract?sid=b4d2d171-a9b2-4f05-a090-2eac3427ffcc

http://www.sciencemag.org/content/347/6226/1100.full



* Thank for citing our paper, 
http://pasj.oxfordjournals.org/content/67/2/23,
An X-ray spectroscopic search for dark matter in the Perseus cluster with Suzaku