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。 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.
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新引力宇宙度规在星系光度和星系团的验证
The first three columns are the original data of Table (1), and the fourth column is the calculated value of Equation (2a). The value of the third column is smaller than that of the fourth colum
S3.6µm µJy
Z
logL3.6B [Lsun]
logL3.6N [Lsun]
46.17
0.439
9.56
9.9471
10.26
0.549
9.04
9.4920
9.58
0.300
8.60
8.9297
94.89
0.854
10.23
10.8572
14.48
0.923
9.49
10.1126
43.12
1.280
10.24
10.6656
15.55
0.521
9.23
9.2620
17.33
0.914
9.55
10.1815
79.40
0.242
9.23
9.6260
155.99
0.107
8.92
9.2431
576.70
0.607
10.78
11.3315
726.35
0.197
10.12
10.4199
74.66
3.571
11.55
12.3900
27.26
3.130
10.87
11.7469
14.27
4.346
10.81
12.0214
6.87
3.111
10.24
11.1393
6.33
0.158
7.38
8.1959
18.19
4.154
10.88
12.0409
43.91
3.989
11.16
12.3496
6.99
0.138
7.80
8.1158
13.53
1.118
9.62
10.2624
11.55
1.109
9.55
10.1858
99.29
0.507
9.99
10.4056
86.90
1.032
10.37
10.9940
163.41
0.033
7.93
8.2398
76.34
0.282
9.46
9.7756
17.95
0.871
9.56
10.1508
11.82
3.111
10.05
11.3735
96.62
0.219
9.23
9.6571
8.03
0.995
9.28
9.9282
表1. 表中前3列是表(1)原数据,4列是方程(2a)计算值。3列值小于4列值
其中新引力宇宙度规的光度距离是
太阳光度,宇宙视界是上世纪定出,约为
The first three columns are the original data of Table (2), and the fourth column is the calculated value of Equation (2a). The value of the third column is larger than that of the fourth colum
S3.6µm µJy
Z
logL3.6B [Lsun]
logL3.6N [Lsun]
19.76
0.340
9.74
9.3538
4.08
0.400
9.32
8.8114
19.30
0.318
9.46
9.2849
2712.74
0.054
10.30?
10.5877
15.03
0.252
9.48
8.9729
15.12
0.402
9.89
9.3847
14.07
0.326
9.59
9.1694
43.12
0.368
10.02
9.7621
22.41
0.534
10.05
9.8067
9.40
0.334
9.44
9.0155
7.75
0.217
8.96
8.5588
166.84
0.168
10.11
9.6648
264.35
0.062
9.42
8.9979
53.81
0.302
10.05
9.6850
386.48
0.134
10.06
9.8328
25.90
0.694
9.26?
10.1042
77.98
0.112
9.45
8.9817
50.78
0.306
10.11
9.6713
6.92
0.620
10.15
9.4295
371.48
0.216
10.57
10.2314
2658.21
0.012
8.96
8.538
46.17
0.144
9.41
8.9713
14.48
0.288
9.44
9.0720
22.41
0.534
10.50
9.8053
9.40
0.334
9.44
9.0141
28.17
0.188
9.42
8.988
155.99
0.050
8.99
8.5806
22.45
0.294
9.66
9.2805
10.13
0.294
9.32
8.9349
99.29
0.188
9.98
9.5359
表2. 表中前3列是表(2)原数据,4列是方程(2a)计算值。3列值大于4列值
表中的?表示原文计算有错,表(1)的光度距离比表(2)小。The ? in the table indicates that there are some mistakes with the calculation in original literature, Value of luminosity distance in Table (1) is small than Table (2).
黄 洵. 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[J]. 天文与天体物理, 2016, 04(04): 69-80. http://dx.doi.org/10.12677/AAS.2016.44008
参考文献 (References)References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.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.xRowan-Robinson, M., Gonzalez-Solares, E., Vaccari, M. and Marchetti, L. (2013) Revised SWIRE Photometric Redshifts. MNRAS, 428, 1959. http://lanl.arxiv.org/abs/1210.3471v1Marchetti, 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/stv2717Binney, 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.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/1301.3177v1Symeonidis, 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