宇宙几何学初步应用—天体的光度和绝对星等等价不变性的证明
Primary Application of Cosmic Geometry—Proof of Equivalence and Invariant of Astronomical Object’s Luminosity and Absolute Magnitude
摘要: 宇宙几何学是广义相对论导出宇宙均匀引力几何,红移Z > 0.0041的1个天体亮度(通量密度或视星等)是距离的变量;其对应光度或绝对星等是不随距离变化的变量,基础教材仅有以上说,没有数学推导和验证普适性的文献,下面给予严密数学推导和验证(光度和绝对星等是等价不变性)其普适性,并用宇宙均匀引力几何和中心引力几何结合验证引力透镜星系质量计算的普适性。以上的验证是以星系观测最基本数据为依据,证明宇宙几何学的普适性。
Abstract: Cosmic geometry is cosmic even gravity geometry derived by General Relativity. When redshift Z > 0.0041, one astronomical object lightness (flux density or apparent magnitude) is distance’s vari-able and its corresponding luminosity or absolute magnitude is the variable that doesn’t change as distance varies. Above is presented as theory in basic textbook, but without literature of mathe-matical derivation and validation for its universality. The following is the strict mathematical de-rivation and validation for its universality (Luminosity and absolute magnitude is equivalent and invariant). And universality of gravitational lens galaxy mass’s calculation is validated by using cosmic even gravity geometry and central gravity geometry. Validation above is based on basic data from observation of galaxy, which can prove the universality of cosmic geometry.
文章引用:黄洵. 宇宙几何学初步应用—天体的光度和绝对星等等价不变性的证明[J]. 天文与天体物理, 2018, 6(3): 58-74. https://doi.org/10.12677/AAS.2018.63005

参考文献

[1] 黄洵. 新引力宇宙度规计算星系质量和宇宙物质密度的新分析[J]. 天文与天体物理, 2018, 6(1): 11-27. [Google Scholar] [CrossRef
[2] 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 [Google Scholar] [CrossRef
[3] 黄洵. 星系的近似等光度概率和光度图的线性统计分析[J]. 天文与天体物理, 2018, 6(2): 29-46. [Google Scholar] [CrossRef
[4] Conselice, C.J., Wilkinson, A., Duncan, K. and Mortlock, A. (2016) The Evolution of Galaxy Number Density AT Z < 8 AND its Implications. arXiv:1607.03909v2.
http://lanl.arxiv.org/pdf/1607.03909v2
[5] Weinberg, S., 著. 宇宙学[M]. 向守平, 译. 北京: 中国科技大学出版社, 2013: 324-354.
[6] van der Wel, A., van de Ven, G., et.al. (2018) Discovery of a Quadruple Lens in Candels with a Record Lens Redshift z = 1.53. 1309.2826.
http://lanl.arxiv.org/pdf/1309.2826
[7] Dahle, H., Gladders, M.D., Sharon, K., et.al. (2015) Time Delay Measurements for The Cluster-Lensed Sextuple Quasar SDSS J2222+2745 1505.06187.
http://lanl.arxiv.org/pdf/1505.06187
[8] Kratzer, R.M., Richards, G.T., et al. (2011) Analyzing the Flux Anomalies of the Large-Separation Lensed Quasar SDSS J1029+2623 1008.2315.
http://lanl.arxiv.org/pdf/1008.2315
[9] Oguri, M., Schrabback, T., Jullo, E., et al. (2013) The Hidden Fortress: Structure and Substructure of the Complex Strong Lensing Cluster SDSS J1029+2623. Monthly Notices of the Royal Astronomical Society, 429, 482-493.
http://mnras.oxfordjournals.org/content/429/1/482
[10] Oguri, M., Inada, N., et al. (2004) Observations and Theoretical Implica-tions of the Large-Separation Lensed Quasar SDSS J1004+4112. The Astrophysical Journal, 605, 78-97.
[11] Fohlmeister, J., Kochanek, C.S., et al. (2013) A Two-Year Time Delay for the Lensed Quasar SDSS J1029+2623. The Astrophysical Journal, 764, 186.
[12] Suyu, S.H., Marshall, P.J., Auger, M.W., et al. (2010) Dissecting the Gravitational Lens B1608+656. II. Precision Measurements of the Hubble Constant, Spatial Curvature, and the Dark Energy Equation of State. The Astrophysical Journal, 711, 201-221.
[13] Kochanek, C.S., Morgan, N.D., et al. (2006) The Time Delays of Gravitational Lens HE 0435-1223: An Early-Type Galaxy with a Rising Rotation Curve. The Astrophysical Journal, 640, 47-61.
http://iopscience.iop.org/article/10.1086/499766/pdf
[14] Dahle, H., Gladders, M.D., Sharon, K., et al. (2013) SDSS J2222+2745: A Gravitationally Lensed Sextuple Quasar with a Maximum Image Separation of 15".1 Discovered in the Sloan Giant Arcs Survey. The Astrophysical Journal, 773, 146.
https://arxiv.org/pdf/1211.1091.pdf
[15] Geach, J.E., More, A., Verma, A., Marshall, P.J., et al. (2015) The Red Radio Ring: A Gravitationally Lensed Hyperluminous Infrared Radio Galaxy at z = 2.553 Discovered through Citizen Science. Monthly Notices of the Royal Astronomical Society, MN LATEX style file v2.2, 1503.05824.
http://xxx.lanl.gov/pdf/1503.05824
[16] Poindexter, S., Morgan, N., Kochanek, C.S. and Falco, E.E. (2007) Mid-IR Observa-tions and a Revised Time Delay for the Gravitational Lens System Quasar HE 1104-1805 0612045. The Astrophysical Journal, 660, 146Y151.
http://lanl.arxiv.org/pdf/astro-ph/0612045
[17] 黄洵. 两种宇宙学模型的延时新分析[EB/OL]. 中科院. 科学智慧火花.
http://idea.cas.cn/viewdoc.action?docid=53282
[18] 黄洵. 新引力宇宙度规与观测数椐部分验证[EB/OL]. 中科院. 科学智慧火花.
http://idea.cas.cn/viewdoc.action?docid=40475