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We investigate the gravitational Higgs mechanism in the inspiraling scalarized neutron star-white dwarf (NS-WD) binaries, whose dynamics are described by the scalar-tensor theory. Because of the difference in binding energy of NS and WD, the orbital decay of scalarized NS-WD system actually sources an emission of dipolar gravitational scalar radiation, in addition to the tensor gravitational waves, which breaks the Lorentz invariance constructed in the framework of general relativity. The resulted gravitational scalar radiation field obtains a scalar-energy-density-dependent effective mass, arising from a gravitational scalar potential that consists of a monotonically decreasing self-interactions of gravitational scalar field and an increasing exponential coupling between the scalar field and the NS/WD matter. Owing to a thin-ring-orbit effect, the gravitational interactions encoded by the massive scalar field are screened in the region of binary orbit, with high density of stars’ scalar energy, which gives us the estimation for scalar masses of about 10−21 eV/c2 and leads to a Yulkawa-like correction to the Newtonian potential of the binary system. We demonstrate that the radiated gravitational tensor waves, propagating in the Yukawa type of potential, gain a scalar-background-dependent mass term of the order of 10−23 eV/c2.
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篇名 Gravitational Higgs Mechanism in Inspiraling Scalarized NS-WD Binary
来源期刊 天文学与天体物理学国际期刊(英文) 学科 地球科学
关键词 Higgs Mechanism GRAVITATIONAL Graviton SCALARIZATION NS-WD BINARY Inspiraling
年,卷(期) 2017,(3) 所属期刊栏目
研究方向 页码范围 202-212
页数 11页 分类号 P1
字数 语种
DOI
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节点文献
Higgs
Mechanism
GRAVITATIONAL
Graviton
SCALARIZATION
NS-WD
BINARY
Inspiraling
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研究去脉
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期刊影响力
天文学与天体物理学国际期刊(英文)
季刊
2161-4717
武汉市江夏区汤逊湖北路38号光谷总部空间
出版文献量(篇)
333
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0
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0
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