空间引力波天线DECIGO和B-DECIGO

S. Kawamura
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引用次数: 61

摘要

DECIGO是日本未来的空间引力波探测器,旨在增强引力波天文学。DECIGO在0.1 Hz至10 Hz的频率范围内工作,在探测包括原始引力波(PGWs)在内的各种来源的引力波信号方面发挥着至关重要的作用。DECIGO的概念前设计特点是由三个航天器组成的集群,每个航天器都配备了激光器和浮动镜,能够精确测量引力波。然而,最近我们对PGWs上限的理解取得了进展,这就需要对DECIGO的设计进行更新。更新后的设计旨在显著提高DECIGO的灵敏度。此外,为了准备DECIGO,计划发射一个名为B-DECIGO的小型版本,以测试各种技术并实现重要的科学目标。DECIGO设计的不断发展和更新表明,它有可能彻底改变引力波天文学,并为重大的科学发现做出贡献。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Space gravitational wave antenna DECIGO and B-DECIGO
DECIGO is a future Japanese gravitational wave detector in space, designed to enhance gravitational wave astronomy. Operating within a frequency range of 0.1 Hz to 10 Hz, DECIGO plays a vital role in detecting gravitational wave signals from various sources, including primordial gravitational waves (PGWs). The pre-conceptual design of DECIGO features a cluster of three spacecraft, each equipped with lasers and floating mirrors, enabling precise measurements of gravitational waves. However, recent advancements in our understanding of the upper limit of PGWs have necessitated an update to DECIGO's design. The updated design aims to significantly improve DECIGO's sensitivity. Additionally, in preparation for DECIGO, a smaller version called B-DECIGO is planned for launch to test various technologies and achieve important scientific objectives. The ongoing development and updates in DECIGO's design demonstrate its potential to revolutionize gravitational wave astronomy and contribute to significant scientific discoveries.
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