Shortcut in codimension-2 brane cosmology in light of GW170817

被引:6
|
作者
Lin, Zi-Chao [1 ,2 ,3 ]
Yu, Hao [4 ]
Liu, Yu-Xiao [1 ,2 ,3 ,5 ]
机构
[1] Lanzhou Univ, Lanzhou Ctr Theoret Phys, Sch Phys Sci & Technol, Key Lab Theoret Phys Gansu Prov, Lanzhou 730000, Peoples R China
[2] Lanzhou Univ, Inst Theoret Phys, Lanzhou 730000, Peoples R China
[3] Lanzhou Univ, Res Ctr Gravitat, Lanzhou 730000, Peoples R China
[4] Chongqing Univ, Phys Dept, Chongqing 401331, Peoples R China
[5] Lanzhou Univ, Key Lab Magnetism & Magnet Minist Educ, Lanzhou 730000, Peoples R China
来源
EUROPEAN PHYSICAL JOURNAL C | 2023年 / 83卷 / 03期
基金
中国国家自然科学基金;
关键词
QUANTUM-THEORY; DIMENSIONS; SPACE; HIERARCHY; GRAVITY;
D O I
10.1140/epjc/s10052-023-11328-x
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
In this paper, our universe is regarded as a codimension-2 brane embedded in a noncompact six dimensional Anti-de Sitter (AdS) spacetime. We derive the gravitational horizon radius on the brane under the low energy approximation, which reflects how the extra dimensions cause the shortcut effect of gravitational waves (GWs). We also study the time delay between a GW signal and an electromagnetic (EM) wave signal in the low-redshift limit by combining with the joint observations of GW170817 and GRB 170817A, which gives an upper limit to the AdS(6) radius as l(2) ? 3.84 Mpc(2). For a high-redshift source, the time delay is converted into the discrepancy between the source redshift derived from the GW signal and the one derived from the EM counterpart. It is found that if one expects to detect the EM counterpart of a high-redshift GW event within a reasonable observation time, it requires a stronger constraint on the AdS6 radius. Our research shows that the AdS6 radius should satisfy l(2) ? 0.02 Mpc(2) for the DECIGO and BBO.
引用
收藏
页数:14
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