天文与天体物理  >> Vol. 4 No. 4 (October 2016)

新引力宇宙度规在星系光度和星系团的验证
Validation of New Gravity Universal Metric in Galaxy Luminosity and Galaxy Groups and Clusters

DOI: 10.12677/AAS.2016.44008, PDF, HTML, XML,  被引量 下载: 1,399  浏览: 3,329 

作者: 黄 洵:广东省梅州市兴宁市宁江中学,广东 兴宁

关键词: 红外通量密度宇宙视界光度图星系团Infrared Flux Density Universal Horizon Luminosity Diagram Galaxy Groups and Clusters

摘要: 新引力宇宙度规导出新光度和光度距离方程,可以绘出全部红移的光度距离图,是斜率为0.5的直线簇,能对每个光度在图中精确表述。光度(L–L)图的点坐标集中在对角线两旁,紧凑有规律分布,全部红移绘出图。标准宇宙学没有这样的图。计算分析高红移星系团应该是星系长城局域。星系所有观测的物理量都受到宇宙基本均匀的引力效应,随红移值增大宇宙基本均匀引力增强。下面讨论中只有一个宇宙视界恆量,不用暗能量可以分析星系的全红移的光度距离图。
Abstract: With the new cosmic gravity metric, the author gets the new equation of the new luminosity and the luminosity distance to draw the luminosity distance diagram of all the redshifts, which is a line cluster with slope = 0.5. Every luminosity can be shown accurately in this diagram. Point coordinates of luminosity’s diagram (L-L) gather on both sides of diagonal closely and regularly. All the redshifts can be drawn into diagram. There isn’t any diagram like this in standard cosmology. Through calculation and analysis, we can learn that galaxy groups and clusters of high redshift should be the Great Wall of galaxies. All physical quantities in the galaxy are influenced by basically well-distributed gravity effect in the universe and it increases as the redshift’s value increases. In the following discussion, there is only one cosmic horizon constant and all the physical quantities observed on the galaxy with all redshifts can be analyzed without dark energy.

文章引用: 黄洵. 新引力宇宙度规在星系光度和星系团的验证[J]. 天文与天体物理, 2016, 4(4): 69-80. http://dx.doi.org/10.12677/AAS.2016.44008

参考文献

[1] 何香涛. 观测宇宙学[M]. 第二版, 北京: 北京师范大学出版社, 2007: 69.
[2] Rowan-Robinson, M., Babbedge, T., Oliver, S., et al. (2008) Photometric Redshifts in the SWIRE Survey. MNRAS, 386, 697-714. http://dx.doi.org/10.1111/j.1365-2966.2008.13109.x
[3] Rowan-Robinson, M., Gonzalez-Solares, E., Vaccari, M. and Marchetti, L. (2013) Revised SWIRE Photometric Redshifts. MNRAS, 428, 1959. http://lanl.arxiv.org/abs/1210.3471v1
[4] Marchetti, L., Vaccari, M., Franceschini, A., et al. (2015) The HerMES Submillimetre Local and Low-Redshift Luminosity Functions. MNRAS, 456, 1999-2023. http://lanl.arxiv.org/abs/1511.06167v1 http://dx.doi.org/10.1093/mnras/stv2717
[5] Binney, J. and Merrifield, M., 著. 星系天文学[M]. 赵刚, 陈玉琴, 等, 译. 北亰: 中国科学技术出版社, 2004: 46, 423.
[6] Inger, J. and Chiboucas, K. (2013) Stellar Populations and Evolution of Early-type Cluster Galaxies: Constraints Fromoptical Imagingand Spectroscopyof z=0.5-0.9 Galaxy Clusters. Astronomical Journal, 145, Article ID: 77. http://lanl.arxiv.org/abs/1301.3177v1
[7] Symeonidis, M., Vaccari, M., Berta, S., Page, M.J., et al. (2013) The Herschel Census of Infrared SEDs through Cosmic Time. Oxford Journals Science & Mathematics MNRAS, 431, 2317-2340. http://lanl.arxiv.org/abs/1302.4895v1