Is GW151226 really a gravitational wave signal?

Zhe Chang; Chao-Guang Huang; Zhi-Chao Zhao

doi:10.1088/1674-1137/41/2/025001

Chinese Physics C> 2017, Vol. 41> Issue(2) : 025001 DOI: 10.1088/1674-1137/41/2/025001

Is GW151226 really a gravitational wave signal?

Zhe Chang ^1,2,, ,
Chao-Guang Huang ^1,2,, ,
Zhi-Chao Zhao ^1,2,,

1.
Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China
2.
School of Physics, University of Chinese Academy of Sciences, Beijing 100049, China

Abstract
HTML
Reference
Related

PDF

Abstract：
Recently, the LIGO Scientific Collaboration and Virgo Collaboration published the second observation of a gravitational wave, GW151226[Phys. Rev. Lett. 116, 241103 (2016)], from a binary black hole coalescence with initial masses about 14 M_⊙ and 8 M_⊙. They claimed that the peak gravitational strain was reached at about 450 Hz, the inverse of which is longer than the average time a photon stays in the Fabry-Perot cavities in the two arms. In this case, the phase-difference of a photon in the two arms due to the propagation of a gravitational wave does not always increase as the photon stays in the cavities. It might even be cancelled to zero in extreme cases. When the propagation effect is taken into account, we find that the claimed signal GW151226 almost disappears.
- gravitational wave ,
- gravitational wave detector ,
- LIGO

References

[1]	B. P. Abbott et al, Phys. Rev. Lett., 116:061102(2016)
[2]	J. A. Orosz et al, Nature, 449:872-875(2007)
[3]	B. P. Abbott et al, Phys. Rev. Lett., 116:241103(2016)
[4]	For example, see:E. D. Black and R. N. Gutenkunst, Am. J. Phys., 71:365-378(2003)
[5]	B. Allen, W. G. Anderson, P. R. Brady, D. A. Brown, and J. D. E. Creighton, Phys. Rev. D, 85:122006(2012)
[6]	Rakhmanov, M., J. D. Romano, and John T. Whelan, Class.Quantum Grav., 25.18:184017(2008)
[7]	K. S. Thorne, in Three hundred years of gravitation, edited by S. W. Hawking and W. Israel, (Cambridge University Press, Cambridge, 1987), p.330
[8]	E.D. Black and R.N.Gutenkunst, Am. J. Phys., 69:79-87(2001)
[9]	https:\\losc.ligo.org\tutorials\
[10]	Chang Z, Huang CG, Zhao ZC, Sci. China-Phys. Mech. Astro., 59:100421(2016)
[11]	Abbott, B.P. and LIGO Scientific Collaboration, arXiv:1602. 03845, 2016

[1]	Reggie C. Pantig , Ali Övgün . Imprints of a gravitational wave through the weak field deflection of photons. Chinese Physics C, 2024, 48(8): 085104. doi: 10.1088/1674-1137/ad4e25
[2]	Lu Feng , Tao Han , Jing-Fei Zhang , Xin Zhang . Prospects for weighing neutrinos in interacting dark energy models using joint observations of gravitational waves and γ-ray bursts. Chinese Physics C, 2024, 48(9): 095104. doi: 10.1088/1674-1137/ad5ae4
[3]	He-Xu Zhang , Shinya Matsuzaki , Hiroyuki Ishida . Gravitational wave footprints from Higgs-portal scalegenesis with multiple dark chiral scalars. Chinese Physics C, 2024, 48(4): 045106. doi: 10.1088/1674-1137/ad2b4f
[4]	Tian-Yang Sun , Chun-Yu Xiong , Shang-Jie Jin , Yu-Xin Wang , Jing-Fei Zhang , Xin Zhang . Efficient parameter inference for gravitational wave signals in the presence of transient noises using temporal and time-spectral fusion normalizing flow. Chinese Physics C, 2024, 48(4): 045108. doi: 10.1088/1674-1137/ad2a5f
[5]	Shang-Jie Jin , Shuang-Shuang Xing , Yue Shao , Jing-Fei Zhang , Xin Zhang . Joint constraints on cosmological parameters using future multi-band gravitational wave standard siren observations. Chinese Physics C, 2023, 47(6): 065104. doi: 10.1088/1674-1137/acc8be
[6]	Bum-Hoon Lee , Wonwoo Lee , Dong-han Yeom , Lu Yin . Gravitational waves from the vacuum decay with LISA. Chinese Physics C, 2022, 46(7): 075101. doi: 10.1088/1674-1137/ac5d2a
[7]	Wenfeng Cui , Fei Huang , Jing Shu , Yue Zhao . Stochastic gravitational wave background from PBH-ABH mergers. Chinese Physics C, 2022, 46(5): 055103. doi: 10.1088/1674-1137/ac4cab
[8]	Ligong Bian , Wei Cheng , Huai-Ke Guo , Yongchao Zhang . Cosmological implications of a B − L charged hidden scalar: leptogenesis and gravitational waves. Chinese Physics C, 2021, 45(11): 113104. doi: 10.1088/1674-1137/ac1e09
[9]	Wei Chao , Wen-Feng Cui , Huai-Ke Guo , Jing Shu . Gravitational wave imprint of new symmetry breaking. Chinese Physics C, 2020, 44(12): 123102. doi: 10.1088/1674-1137/abb4cb
[10]	Zhi-Chao Zhao , Hai-Nan Lin , Zhe Chang . The prospects of using gravitational waves for constraining the anisotropy of the Universe. Chinese Physics C, 2019, 43(7): 075102. doi: 10.1088/1674-1137/43/7/075102
[11]	Yanyan Bu , Shu Lin . Holographic magnetized chiral density wave. Chinese Physics C, 2018, 42(11): 114104. doi: 10.1088/1674-1137/42/11/114104
[12]	Andrea Addazi , Antonino Marcianò . Limiting majoron self-interactions from gravitational wave experiments. Chinese Physics C, 2018, 42(2): 023105. doi: 10.1088/1674-1137/42/2/023105
[13]	Xin Li , Li Tang , Hai-Nan Lin , Li-Li Wang . Testing the variation of the fine structure constant with strongly lensed gravitational waves. Chinese Physics C, 2018, 42(9): 095104. doi: 10.1088/1674-1137/42/9/095104
[14]	Zhe Chang , Chao-Guang Huang , Zhi-Chao Zhao . Motion of photons in a gravitational wave background. Chinese Physics C, 2017, 41(9): 093108. doi: 10.1088/1674-1137/41/9/093108
[15]	WU Yang , XU Zhou , LI Zheng-Hong , MA Qiao-Sheng , TANG Chuan-Xiang . High efficiency X-band relativistic backward wave oscillator with non-uniform slow wave structures. Chinese Physics C, 2012, 36(8): 750-752. doi: 10.1088/1674-1137/36/8/011
[16]	ZHANG Xu-Ning . Constraints of gravitational baryo/leptogenesis on Cardassian expansion. Chinese Physics C, 2011, 35(10): 920-924. doi: 10.1088/1674-1137/35/10/006
[17]	WANG Guo-Li , ZHANG Jin-Mei , WANG Zhi-Hui . Relativistic studies of the decay constants of S wave and P wave mesons. Chinese Physics C, 2010, 34(2): 274-276. doi: 10.1088/1674-1137/34/2/024
[18]	A. Sarantsev . Bonn-Gatchina partial wave analysis. Chinese Physics C, 2009, 33(12): 1085-1092. doi: 10.1088/1674-1137/33/12/007
[19]	MA Qiao-Sheng , ZHOU Chuan-Min , WU Yong . Theoretical investigation of a backward wave oscillator. Chinese Physics C, 2008, 32(4): 290-293. doi: 10.1088/1674-1137/32/4/010
[20]	HUANG Chao-Guang , ZHANG Hai-Qing , GUO Han-Ying . A new gravitational model for dark energy. Chinese Physics C, 2008, 32(9): 687-691. doi: 10.1088/1674-1137/32/9/002

Access

Get Citation

Zhe Chang, Chao-Guang Huang and Zhi-Chao Zhao. Is GW151226 really a gravitational wave signal?[J]. Chinese Physics C, 2017, 41(2): 025001. doi: 10.1088/1674-1137/41/2/025001

Zhe Chang, Chao-Guang Huang and Zhi-Chao Zhao. Is GW151226 really a gravitational wave signal?[J]. Chinese Physics C, 2017, 41(2): 025001. doi: 10.1088/1674-1137/41/2/025001 shu

RIS(for EndNote,Reference Manager,ProCite)

BibTex

Txt

Milestone

Received: 2016-08-13

Fund

Supported by National Natural Science Foundation of China (11275207, 11375203, 11690022, 11675182) and Strategic Priority Research Program of the Chinese Academy of Sciences Multi-waveband Gravitational Wave Universe (XDB23040000)

Article Metric

Article Views(1564)
PDF Downloads(29)
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

Is GW151226 really a gravitational wave signal?

Corresponding author: Zhe Chang,

Corresponding author: Chao-Guang Huang,

Corresponding author: Zhi-Chao Zhao,

1. Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China

2. School of Physics, University of Chinese Academy of Sciences, Beijing 100049, China

Received Date: 2016-08-13

Available Online: 2017-02-05

Fund Project: Supported by National Natural Science Foundation of China (11275207, 11375203, 11690022, 11675182) and Strategic Priority Research Program of the Chinese Academy of Sciences Multi-waveband Gravitational Wave Universe (XDB23040000)

Abstract: Recently, the LIGO Scientific Collaboration and Virgo Collaboration published the second observation of a gravitational wave, GW151226[Phys. Rev. Lett. 116, 241103 (2016)], from a binary black hole coalescence with initial masses about 14 M_⊙ and 8 M_⊙. They claimed that the peak gravitational strain was reached at about 450 Hz, the inverse of which is longer than the average time a photon stays in the Fabry-Perot cavities in the two arms. In this case, the phase-difference of a photon in the two arms due to the propagation of a gravitational wave does not always increase as the photon stays in the cavities. It might even be cancelled to zero in extreme cases. When the propagation effect is taken into account, we find that the claimed signal GW151226 almost disappears.

HTML

Reference (11)

Is GW151226 really a gravitational wave signal?

Abstract：

References

Access

Article Metrics

Metrics

通讯作者: 陈斌, bchen63@163.com

Email This Article