Impact factor of Chinese Physics C is 3.6 in 2023 Impact factor of Chinese Physics C is 3.6 in 2022 2021 Impact Factor 2.944
Advanced Search
×
近期发现有不法分子冒充我刊与作者联系，借此进行欺诈等不法行为，请广大作者加以鉴别，如遇诈骗行为，请第一时间与我刊编辑部联系确认（《中国物理C》（英文）编辑部电话：010-88235947,010-88236950），并作报警处理。
本刊再次郑重声明：
（1）本刊官方网址为cpc.ihep.ac.cn和https://iopscience.iop.org/journal/1674-1137
（2）本刊采编系统作者中心是投稿的唯一路径，该系统为ScholarOne远程稿件采编系统，仅在本刊投稿网网址（https://mc03.manuscriptcentral.com/cpc）设有登录入口。本刊不接受其他方式的投稿，如打印稿投稿、E-mail信箱投稿等，若以此种方式接收投稿均为假冒。
（3）所有投稿均需经过严格的同行评议、编辑加工后方可发表，本刊不存在所谓的“编辑部内部征稿”。如果有人以“编辑部内部人员”名义帮助作者发稿，并收取发表费用，均为假冒。
                  
《中国物理C》（英文）编辑部
2024年10月30日
Chinese Physics C> 2018, Vol. 42> Issue(7) : 075101 DOI: 10.1088/1674-1137/42/7/075101

Doubly coupled matter fields in massive bigravity

  • 1.

     School of Physics and Astronomy, Sun Yat-sen University, Guangzhou 510275, China

  • 2.

     Research Center for the Early Universe(RESCEU), Graduate School of Science, The University of Tokyo, Tokyo 113-0033, Japan

  • 3.

     Department of Physics, Tokyo Institute of Technology, 2-12-1 Ookayama, Meguro, Tokyo 152-8551, Japan

  • 4.

      Institute for Theoretical Studies, ETH Zurich, Clausiusstrasse 47, 8092 Zurich, Switzerland

  • In the context of massive (bi-)gravity, non-minimal matter couplings have been proposed. These couplings are special in the sense that they are free of the Boulware-Deser ghost below the strong coupling scale and can be used consistently as an effective field theory. Furthermore, they enrich the phenomenology of massive gravity. We consider these couplings in the framework of bimetric gravity and study the cosmological implications for background and linear tensor, vector, and scalar Previous works have investigated special branches of solutions. Here we perform a complete perturbation analysis for the general background equations of motion, completing previous analyses.
      PCAS:
  • 加载中

  • References

    [1] P. A. R. Ade et al (Planck), (2015), arXiv: 1506.07135 [astroph.CO]
    [2] P. A. R. Ade et al (Planck), (2015), arXiv: 1502.01589 [astroph.CO]
    [3] P. Ade et al (Planck), (2015), arXiv: 1502.02114 [astro-ph.CO]
    [4] L. Amendola et a. (Euclid Theory Working Group), Living Rev. Rel., 16: 6 (2013), arXiv: 1206.1225 [astro-ph.CO]
    [5] S. Weinberg, Rev. Mod. Phys., 61: 1 (1989)
    [6] G. W. Horndeski, Int. J. Theor. Phys., 10: 363 (1974)
    [7] A. Nicolis, R. Rattazzi, and E. Trincherini, Phys. Rev. D, 79:064036 (2009), arXiv: 0811.2197 [hep-th]
    [8] C. Deffayet, G. Esposito-Farese, and A. Vikman, Phys. Rev. D, 79: 084003 (2009), arXiv: 0901.1314 [hep-th]
    [9] C. Deffayet, S. Deser, and G. Esposito-Farese, Phys. Rev. D, 80: 064015 (2009), arXiv: 0906.1967 [gr-qc]
    [10] C. Deffayet, X. Gao, D. Steer, and G. Zahariade, Phys. Rev. D, 84: 064039 (2011), arXiv: 1103.3260 [hep-th]
    [11] A. De Felice and S. Tsujikawa, Phys. Rev. Lett., 105: 111301 (2010), arXiv: 1007.2700 [astro-ph.CO]
    [12] T. Kobayashi, M. Yamaguchi, and J. Yokoyama, Phys. Rev. Lett., 105: 231302 (2010), arXiv: 1008.0603 [hep-th]
    [13] T. Kobayashi, M. Yamaguchi, and J. Yokoyama, Prog. Theor. Phys., 126: 511 (2011), arXiv: 1105.5723 [hep-th]
    [14] X. Gao and D. A. Steer, JCAP, 1112: 019 (2011), arXiv: 1107.2642 [astro-ph.CO]
    [15] X. Gao, JCAP, 1110: 021 (2011), arXiv: 1106.0292 [astroph.CO]
    [16] A. De Felice and S. Tsujikawa, Phys. Rev. D, 84: 083504 (2011), arXiv: 1107.3917 [gr-qc]
    [17] C. de Rham and L. Heisenberg, Phys. Rev. D, 84: 043503 (2011), arXiv: 1106.3312 [hep-th]
    [18] L. Heisenberg, R. Kimura, and K. Yamamoto, Phys. Rev. D, 89: 103008 (2014), arXiv: 1403.2049 [hep-th]
    [19] G. W. Horndeski, J. Math. Phys., 17: 1980 (1976)
    [20] G. Esposito-Farese, C. Pitrou, and J.-P. Uzan, Phys. Rev. D, 81: 063519 (2010), arXiv: 0912.0481 [gr-qc]
    [21] J. Beltran Jimenez, R. Lazkoz, and A. L. Maroto, Phys. Rev. D, 80: 023004 (2009), arXiv: 0904.0433 [astro-ph.CO]
    [22] J. B. Jimenez, A. L. Delvas Froes, and D. F. Mota, Phys. Lett. B, 725: 212 (2013), arXiv: 1212.1923 [astro-ph.CO]
    [23] J. B. Jimnez, R. Durrer, L. Heisenberg, and M. Thorsrud, JCAP, 1310: 064 (2013), arXiv: 1308.1867 [hep-th]
    [24] J. Beltrn Jimnez and T. S. Koivisto, Class. Quant. Grav., 31: 135002 (2014), arXiv: 1402.1846 [gr-qc]
    [25] L. Heisenberg, JCAP, 1405: 015 (2014), arXiv: 1402.7026 [hepth]
    [26] G. Tasinato, JHEP, 04: 067 (2014), arXiv: 1402.6450 [hep-th]
    [27] E. Allys, P. Peter, and Y. Rodriguez, (2015), arXiv: 1511.03101 [hep-th]
    [28] M. Fierz and W. Pauli, Proc. Roy. Soc. Lond. A, 173: 211 (1939)
    [29] H. van Dam and M. Veltman, Nucl. Phys. B, 22: 397 (1970)
    [30] V. Zakharov, JETP Lett., 12: 312 (1970)
    [31] A. Vainshtein, Phys. Lett. B, 39: 393 (1972)
    [32] D. G. Boulware and S. Deser, Phys. Rev. D, 6: 3368 (1972)
    [33] C. de Rham and G. Gabadadze, Phys. Rev. D, 82: 044020 (2010), arXiv: 1007.0443 [hep-th]
    [34] C. de Rham, G. Gabadadze, and A. J. Tolley, Phys. Rev. Lett., 106: 231101 (2011), arXiv: 1011.1232 [hep-th]
    [35] S. Hassan and R. A. Rosen, JHEP, 1107: 009 (2011), arXiv: 1103.6055 [hep-th]
    [36] S. Hassan and R. A. Rosen, Phys. Rev. Lett., 108: 041101 (2012), arXiv: 1106.3344 [hep-th]
    [37] S. Hassan and R. A. Rosen, JHEP, 1202: 126 (2012), arXiv: 1109.3515 [hep-th]
    [38] C. de Rham, L. Heisenberg, and R. H. Ribeiro, Phys. Rev. D, 88: 084058 (2013), arXiv: 1307.7169 [hep-th]
    [39] C. de Rham, L. Heisenberg, and R. H. Ribeiro, Class. Quant. Grav., 32: 035022 (2015), arXiv: 1408.1678 [hep-th]
    [40] J. Noller and S. Melville, JCAP, 1501: 003 (2015), arXiv: 1408.5131 [hep-th]
    [41] L. Heisenberg, Class. Quant. Grav., 32: 105011 (2015), arXiv: 1410.4239 [hep-th]
    [42] C. de Rham, L. Heisenberg, and R. H. Ribeiro, Phys. Rev. D, 90: 124042 (2014), arXiv: 1409.3834 [hep-th]
    [43] Q.-G. Huang, R. H. Ribeiro, Y.-H. Xing, K.-C. Zhang, and S.-Y. Zhou, Phys. Lett. B, 748: 356 (2015), arXiv: 1505.02616 [hep-th]
    [44] L. Heisenberg, Phys. Rev. D, 92: 023525 (2015), arXiv: 1505.02966 [hep-th]
    [45] S. Melville and J. Noller, (2015), arXiv: 1511.01485 [hep-th]
    [46] K. Hinterbichler and R. A. Rosen, Phys. Rev. D, 92: 024030 (2015), arXiv: 1503.06796 [hep-th]
    [47] C. de Rham and A. J. Tolley, Phys. Rev. D, 92: 024024 (2015), arXiv: 1505.01450 [hep-th]
    [48] A. De Felice, A. E. Gmrkolu,L. Heisenberg, and S. Mukohyama, (2015), arXiv: 1509.05978 [hep-th]
    [49] A. Emir Gmrkolu,L. Heisenberg, and S. Mukohyama, JCAP, 1502: 022 (2015), arXiv: 1409.7260 [hep-th]
    [50] A. R. Solomon, J. Enander, Y. Akrami, T. S. Koivisto, F. Knnig, and E. Mrtsell, JCAP, 1504: 027 (2015), arXiv: 1409.8300 [astro-ph.CO]
    [51] X. Gao and D. Yoshida, Phys. Rev. D, 92: 044057 (2015), arXiv: 1412.8471 [hep-th]
    [52] D. Comelli, M. Crisostomi, K. Koyama, L. Pilo, and G. Tasinato, JCAP, 1504: 026 (2015), arXiv: 1501.00864 [hep-th]
    [53] A. E. Gumrukcuoglu, L. Heisenberg, S. Mukohyama, and N. Tanahashi, JCAP, 1504: 008 (2015), arXiv: 1501.02790 [hep-th]
    [54] M. Lagos and J. Noller, (2015), arXiv: 1508.05864 [gr-qc]
    [55] L. Heisenberg, JCAP, 1511: 005 (2015), arXiv: 1506.00580 [hep-th]
    [56] L. Heisenberg and A. Refregier, (2016), arXiv: 1604.07306 [gr-qc]
    [57] L. Heisenberg and A. Refregier, (2016), arXiv: 1604.07680 [astro-ph.CO]
    [58] L. Blanchet and L. Heisenberg, Phys. Rev. D, 91: 103518 (2015), arXiv: 1504.00870 [gr-qc]
    [59] L. Blanchet and L. Heisenberg, JCAP, 1512: 026 (2015), arXiv: 1505.05146 [hep-th]
    [60] L. Bernard, L. Blanchet, and L. Heisenberg, in Proceedings, 50th Recontres de Moriond Gravitaion : 100 years after GR (2015) pp. 4352, arXiv: 1507.02802 [gr-qc]
    [61] X. Gao and L. Heisenberg, JCAP, 1603: 043 (2016), arXiv: 1601.02180 [hep-th]
    [62] P. Brax, A.-C. Davis, and J. Noller, (2016), arXiv: 1606.05590 [gr-qc]

  • Access

    加载中

Get Citation
Xian Gao and Lavinia Heisenberg. Doubly coupled matter fields in massive bigravity[J]. Chinese Physics C, 2018, 42(7): 075101. doi: 10.1088/1674-1137/42/7/075101
Xian Gao and Lavinia Heisenberg. Doubly coupled matter fields in massive bigravity[J]. Chinese Physics C, 2018, 42(7): 075101.  doi: 10.1088/1674-1137/42/7/075101 shu
Milestone
Received: 2018-04-19
Fund

    Supported by the Chinese National Youth Thousand Talents Program (71000-41180003), JSPS Grant-in-Aid for Scientific Research (15H02082, 25287054, 26610062), L. H. Acknowledges Financial Support from Dr. Max Rssler, the Walter Haefner Foundation and the ETH Zurich Foundation

Article Metric

Article Views(1760)
PDF Downloads(13)
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

  1. 本站搜索
  2. 百度学术搜索
  3. 万方数据库搜索
  4. CNKI搜索

Email This Article

Title:
Email:

Doubly coupled matter fields in massive bigravity

  • 1. School of Physics and Astronomy, Sun Yat-sen University, Guangzhou 510275, China
  • 2. Research Center for the Early Universe(RESCEU), Graduate School of Science, The University of Tokyo, Tokyo 113-0033, Japan
  • 3. Department of Physics, Tokyo Institute of Technology, 2-12-1 Ookayama, Meguro, Tokyo 152-8551, Japan
  • 4.  Institute for Theoretical Studies, ETH Zurich, Clausiusstrasse 47, 8092 Zurich, Switzerland
  • Received Date: 2018-04-19
  • Available Online: 2018-07-05
Fund Project:  Supported by the Chinese National Youth Thousand Talents Program (71000-41180003), JSPS Grant-in-Aid for Scientific Research (15H02082, 25287054, 26610062), L. H. Acknowledges Financial Support from Dr. Max Rssler, the Walter Haefner Foundation and the ETH Zurich Foundation

Abstract: In the context of massive (bi-)gravity, non-minimal matter couplings have been proposed. These couplings are special in the sense that they are free of the Boulware-Deser ghost below the strong coupling scale and can be used consistently as an effective field theory. Furthermore, they enrich the phenomenology of massive gravity. We consider these couplings in the framework of bimetric gravity and study the cosmological implications for background and linear tensor, vector, and scalar Previous works have investigated special branches of solutions. Here we perform a complete perturbation analysis for the general background equations of motion, completing previous analyses.

    HTML

Reference (62)

目录

Link
IOPScience
SCOAP3
arXiv
Chinese Physical Society
Journal information
Introduction
Editorial Board
Others
Subscribe
Contact us
QQ: 1307685413
Tel: +86-010-88235947
Fax: +86-010-88233126
E-mail: cpc@ihep.ac.cn

  • CPC Website

  • IOP Website

  • CPC WeChat

Copyright © Institute of High Energy Physics, Chinese Academy of Sciences, 19B Yuquan Road, Beijing 100049, China 京ICP备05002789号-1

Supported by: Beijing Renhe Information Technology Co. Ltd  E-mail: info@rhhz.net

/

DownLoad:  Full-Size Img  PowerPoint
Return
Return