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arXiv 1402.0053gr-qcastro-ph.IM
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地基引力波天文学中外参数空间的物理激发探索

Physically motivated exploration of the extrinsic parameter space in ground-based gravitational-wave astronomy

V. Raymond, W. M. Farr

摘要:

有效的参数估计是引力波天文学的关键。在紧凑的二进制合并的情况下,高维参数空间需要有效的采样技术-如马尔可夫链蒙特卡罗(MCMC)。许多退化有效地降低了参数空间的维数,并且当已知时,可以使采样算法更有效地与特定问题的改进。我们提出了在本文中的一个简并涉及一个紧凑的二元聚结引力波信号的外部参数的分析描述,当数据从一个三探测器网络(如先进的LIGO/处女座)。我们使用这个新的公式来构建一个跳跃的建议,一个框架的通用采样器,以利用退化。我们显示了MCMC采样器的效率增益的引力波信号从一个紧凑的二进制合并的分析。

英文摘要:

Efficient parameter estimation is critical for Gravitational-Wave astronomy. In the case of compact binary coalescence, the high dimensional parameter space demands efficient sampling techniques - such as Markov chain Monte Carlo (MCMC). A number of degeneracies effectively reduce the dimensionality of the parameter space and, when known, can render sampling algorithms more efficient with problem-specific improvements. We present in this paper an analytical description of a degeneracy involving the extrinsic parameters of a compact binary coalescence gravitational-wave signal, when data from a three detector network (such as Advanced LIGO/Virgo) is available. We use this new formula to construct a jump proposal, a framework for a generic sampler to take advantage of the degeneracy. We show the gain in efficiency for a MCMC sampler in the analysis of the gravitational-wave signal from a compact binary coalescence.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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