Searching for a possible dipole anisotropy in acceleration scale with 147 rotationally supported galaxies

Zhe Chang; Hai-Nan Lin; Zhi-Chao Zhao; Yong Zhou

doi:10.1088/1674-1137/42/11/115103

Chinese Physics C> 2018, Vol. 42> Issue(11) : 115103 DOI: 10.1088/1674-1137/42/11/115103

Searching for a possible dipole anisotropy in acceleration scale with 147 rotationally supported galaxies

Zhe Chang ^1,2 ,
Hai-Nan Lin ³ ,
Zhi-Chao Zhao ^1,2 ,
Yong Zhou ^1,2

1.
Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China
2.
School of Physical Sciences, University of Chinese Academy of Sciences, Beijing 100049, China
3.
Department of Physics, Chongqing University, Chongqing 401331, China

Abstract
HTML
Reference
Related

PDF

Abstract：
We report a possible dipole anisotropy in acceleration scale g_† with 147 rotationally supported galaxies in the local Universe. It is found that a monopole and dipole correction for the radial acceleration relation can better describe the SPARC data set. The monopole term is negligible but the dipole magnitude is significant. It is also found that the dipole correction is mostly induced by anisotropy in the acceleration scale. The magnitude of the ĝ_†-dipole reaches 0.25±0.04, and its direction is aligned to (l,b)=(171.30°±7.18°, -15.41°±4.87°), which is very close to the maximum anisotropy direction from the hemisphere comparison method. Furthermore, a robust check shows that the dipole anisotropy could not be reproduced by an isotropic mock data set. However, it is still premature to claim that the Universe is anisotropic, due to the small data samples and uncertainty in the current observations.
- galaxies:kinematics and dynamics ,
- galaxies:fundamental parameters ,
- large-scale structure of Universe

References

[1]	S. Weinberg, Cosmology, (Oxford, UK:Oxford University Press, 2008)
[2]	C. L. Bennett et al (WMAP), Astrophys. J. Suppl., 208:20 (2013)
[3]	G. Hinshaw et al (WMAP), Astrophys. J. Suppl., 208:19 (2013)
[4]	P. A. R. Ade et al (Planck), Astron. Astrophys., 571:A16 (2014)
[5]	P. A. R. Ade et al (Planck), Astron. Astrophys., 594:A13 (2016)
[6]	D. Hutsemekers, R. Cabanac, H. Lamy, and D. Sluse, Astron. Astrophys., 441:915 (2005)
[7]	A. Kashlinsky, F. Atrio-Barandela, H. Ebeling, A. Edge, and D. Kocevski, Astrophys. J., 712:L81 (2010)
[8]	H. A. Feldman, R. Watkins, and M. J. Hudson, Mon. Not. Roy. Astron. Soc., 407:2328 (2010)
[9]	J. K. Webb, J. A. King, M. T. Murphy, V. V. Flambaum, R. F. Carswell, and M. B. Bainbridge, Phys. Rev. Lett., 107:191101 (2011)
[10]	J. A. King, J. K. Webb, M. T. Murphy, V. V. Flambaum, R. F. Carswell, M. B. Bainbridge, M. R. Wilczynska, and F. E. Koch, Mon. Not. Roy. Astron. Soc., 422:3370 (2012)
[11]	A. Mariano and L. Perivolaropoulos, Phys. Rev. D, 86:083517 (2012)
[12]	Z. Chang, X. Li, H.-N. Lin, and S. Wang, Eur. Phys. J. C, 74:2821 (2014)
[13]	Z. Chang and H.-N. Lin, Mon. Not. Roy. Astron. Soc., 446:2952 (2015)
[14]	H.-N. Lin, X. Li, and Z. Chang, Mon. Not. Roy. Astron. Soc., 460:617 (2016)
[15]	V. C. Rubin, W. K. Ford, Jr., and N. Thonnard, Astrophys. J., 225:L107 (1978)
[16]	A. Bosma, Astron. J., 86:1825 (1981)
[17]	A. Tan et al (PandaX-Ⅱ), Phys. Rev. Lett., 117:121303 (2016)
[18]	E. Aprile et al (XENON100), Phys. Rev. D, 94:122001 (2016)
[19]	M. Milgrom, Astrophys. J., 270:365 (1983)
[20]	M. Milgrom, New Astron. Rev., 46:741 (2002)
[21]	M. Milgrom, Mon. Not. Roy. Astron. Soc., 437:2531 (2014)
[22]	K. G. Begeman, A. H. Broeils, and R. H. Sanders, Mon. Not. Roy. Astron. Soc., 249:523 (1991)
[23]	R. A. Swaters, R. H. Sanders, and S. S. McGaugh, Astrophys. J., 718:380 (2010)
[24]	Z. Chang, M.-H. Li, X. Li, H.-N. Lin, and S. Wang, Eur. Phys. J. C, 73:2447 (2013)
[25]	M. Milgrom, in Proceedings, 2nd International Heidelberg Conference on Dark matter in astrophysics and particle physics (DARK 1998):Heidelberg, Germany, July 20-25, 1998 (1998) p. 443-457
[26]	Y. Zhou, Z.-C. Zhao, and Z. Chang, Astrophys. J., 847:86 (2017)
[27]	F. Lelli, S. S. McGaugh, and J. M. Schombert, Astron. J., 152:157 (2016)
[28]	S. S. McGaugh, F. Lelli, and J. M. Schombert, Phys. Rev. Lett., 117:201101 (2016)
[29]	A. Begum and J. N. Chengalur, Astron. Astrophys., 424:509 (2005)
[30]	W. J. G. de Blok, S. S. McGaugh, and J. M. van der Hulst, Mon. Not. Roy. Astron. Soc., 283:18 (1996)
[31]	M. Milgrom, (2016), arXiv:1609.06642
[32]	P. T. Boggs, R. H. Byrd, and R. B. Schnabel, SIAM Journal on Scientific and Statistical Computing, 8:1052 (1987)
[33]	H. Akaike, IEEE Transactions on Automatic Control, 19:716 (1974)
[34]	G. Schwarz, Annals of Statistics, 6:461 (1978)
[35]	A. R. Liddle, Mon. Not. Roy. Astron. Soc., 377:L74 (2007)
[36]	F. Arevalo, A. Cid, and J. Moya, Eur. Phys. J. C, 77:565 (2017)
[37]	H.-N. Lin, X. Li, and Y. Sang, (2017), arXiv:1711.05025
[38]	D. Foreman-Mackey, D. W. Hogg, D. Lang, and J. Goodman, Publications of the Astronomical Society of the Pacific, 125:306 (2013)
[39]	W. Zhao, P.-X. Wu, and Y. Zhang, Int. J. Mod. Phys. D, 22:1350060 (2013)
[40]	Z. Chang, S. Wang, and X. Li, Eur. Phys. J. C, 72:1838 (2012)
[41]	Z. Chang, M.-H. Li, and S. Wang, Phys. Lett. B, 723:257 (2013)
[42]	X. Li, H.-N. Lin, S. Wang, and Z. Chang, Eur. Phys. J. C, 75:181 (2015)
[43]	J. M. Schombert and S. McGaugh, PASA, 31:e011 (2014)
[44]	P.-F. Li, F. Lelli, S. McGaugh, and J. Schormbert, Astron. Astrophys., 615:A3 (2018)

[1]	Li Tang , Hai-Nan Lin , Liang Liu , Xin Li . Consistency of Pantheon+ supernovae with a large-scale isotropic universe. Chinese Physics C, 2023, 47(12): 125101. doi: 10.1088/1674-1137/acfaf0
[2]	Xiaobo Gong , Meirong Tang , Zhaoyi Xu . The possible equation of state of dark matter in low surface brightness galaxies. Chinese Physics C, 2021, 45(10): 105103. doi: 10.1088/1674-1137/ac0f73
[3]	Xin Li , Su-Ping Zhao , Hai-Nan Lin , Yong Zhou . Probing the universality of acceleration scale in modified Newtonian dynamics with SPARC galaxies. Chinese Physics C, 2021, 45(2): 025107. doi: 10.1088/1674-1137/abce53
[4]	Hai-Nan Lin , Yu Sang . Probing the anisotropic distribution of baryon matter in the Universe using fast radio bursts. Chinese Physics C, 2021, 45(12): 125101. doi: 10.1088/1674-1137/ac2660
[5]	Meirong Tang , Zhaoyi Xu , Jiancheng Wang . Observational constraints on Rastall gravity from rotation curves of low surface brightness galaxies. Chinese Physics C, 2020, 44(8): 085104. doi: 10.1088/1674-1137/44/8/085104
[6]	Kui-Xiang Gu , Feng Bing , Wei-Min Pan , Tong-Ming Huang , Qiang Ma , Fan-Bo Meng . Development of fundamental power coupler for C-ADS superconducting elliptical cavities. Chinese Physics C, 2017, 41(6): 067001. doi: 10.1088/1674-1137/41/6/067001
[7]	Xin Li , Hai-Nan Lin . Spatial and temporal variations of the fine-structure constant in the Finslerian universe. Chinese Physics C, 2017, 41(6): 065102. doi: 10.1088/1674-1137/41/6/065102
[8]	A. Sojasi , M. Mohsenzadeh , E. Yusofi . Large angular scale CMB anisotropy from an excited initial mode. Chinese Physics C, 2016, 40(7): 075101. doi: 10.1088/1674-1137/40/7/075101
[9]	YANG Zi-Qin , LU Xiang-Yang , ZHAO Ji-Fei , QUAN Sheng-Wen , LUO Xing , ZHOU Kui , YANG De-Yu . Electromagnetic design and beam dynamics simulation of a new superconducting accelerating structure for extremely low β protons. Chinese Physics C, 2015, 39(10): 107001. doi: 10.1088/1674-1137/39/10/107001
[10]	ZHAO Dong , LI Ming-Hua , WANG Ping , CHANG Zhe . Inflation in de Sitter spacetime and CMB large scale anomaly. Chinese Physics C, 2015, 39(9): 095101. doi: 10.1088/1674-1137/39/9/095101
[11]	HUANG Chao-Guang , LI Lin . Possible supersymmetric kinematics. Chinese Physics C, 2015, 39(9): 093103. doi: 10.1088/1674-1137/39/9/093103
[12]	PANG Dan-Yang . Effects of relativistic kinematics in heavy ion elastic scattering. Chinese Physics C, 2014, 38(2): 024104. doi: 10.1088/1674-1137/38/2/024104
[13]	YE Qing , CHEN Xing , ZHOU Jing , ZHAO Hai-Feng , CHU Wang-Sheng , ZHENG Xu-Sheng , WU Zi-Yu . Local hydrated structure of an Fe²⁺/Fe³⁺ aqueous solution: an investigation using a combination of molecular dynamics and X-ray absorption fine structure methods. Chinese Physics C, 2013, 37(3): 038003. doi: 10.1088/1674-1137/37/3/038003
[14]	XING Hao-Yang , WANG Li , ZHU Jing-Jun , TANG Chang-Jian , YUE Qian . Simulation of large-scale fast neutron liquid scintillation detector. Chinese Physics C, 2013, 37(2): 026003. doi: 10.1088/1674-1137/37/2/026003
[15]	LI Xin , CHANG Zhe . Kinematics in Randers-Finsler geometry and secular increase of the astronomical unit. Chinese Physics C, 2011, 35(10): 914-919. doi: 10.1088/1674-1137/35/10/005
[16]	MO Xiao-Hu . Kinematics of τ two-body decay near τ threshold at BESⅢ. Chinese Physics C, 2010, 34(11): 1671-1679. doi: 10.1088/1674-1137/34/11/001
[17]	N. Suzuki , T. -S. H. Lee . Extraction of resonance parameters from meson production reaction. Chinese Physics C, 2009, 33(12): 1140-1145. doi: 10.1088/1674-1137/33/12/015
[18]	HE Xiao-Tao , REN Zhong-Zhou . Temporal variation of fundamental constants in ²²⁹Th transition. Chinese Physics C, 2008, 32(S2): 162-165.
[19]	Ren Jingru , Lu Suiling , Su Shi , Huo Anxiang , Wang Chengrui , Zhang Naijian , He Mao , Cao Peiyuan , Li Jinyu , Wang Shizhi , Li Guangju , Bai Guangzhi , Liu Zhonghe , Mu Jim , Zhou Wende . A Study of Super High Energy γ-Family Events Through Large-Scale Fe Emulsion Chambers. Chinese Physics C, 1991, 15(S1): 1-6.
[20]	Zheng Xite , Liu Beishu . Calculation of a Fixed Length Fundamental SU(2) Higgs Model. Chinese Physics C, 1990, 14(S1): 45-52.

Access

Figures(1)

Get Citation

Zhe Chang, Hai-Nan Lin, Zhi-Chao Zhao and Yong Zhou. Searching for a possible dipole anisotropy in acceleration scale with 147 rotationally supported galaxies[J]. Chinese Physics C, 2018, 42(11): 115103. doi: 10.1088/1674-1137/42/11/115103

RIS(for EndNote,Reference Manager,ProCite)

BibTex

Txt

Milestone

Received: 2018-07-27

Fund

Supported by National Natural Science Foundation of China (11675182, 11690022, 11603005)

Article Metric

Article Views(1717)
PDF Downloads(20)
Cited by(0)

Policy on re-use

To reuse of subscription content published by CPC, the users need to request permission from CPC, unless the content was published under an Open Access license which automatically permits that type of reuse.

通讯作者: 陈斌, bchen63@163.com

1.
沈阳化工大学材料科学与工程学院沈阳 110142

Searching for a possible dipole anisotropy in acceleration scale with 147 rotationally supported galaxies

Abstract：

References

Access

Article Metrics

Metrics

通讯作者: 陈斌, bchen63@163.com

Email This Article

Searching for a possible dipole anisotropy in acceleration scale with 147 rotationally supported galaxies

HTML

目录