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cover of episode Deciphering Gravitational Waves, with Janna Levin – StarTalk All-Stars

Deciphering Gravitational Waves, with Janna Levin – StarTalk All-Stars

2024/12/20
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Janna Levin
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Rainer Weiss
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Janna Levin:介绍Rainer Weiss及其在LIGO项目中的贡献,并强调引力波探测的重要性以及公众对这一发现的反应。她还将LIGO比作宇宙录音设备,并与Rainer Weiss探讨了引力波的本质以及探测的挑战。 Matt Kirshen:作为主持人,他与Janna Levin和Rainer Weiss一起讨论了引力波的相关话题,并提出了一些有趣的问题,活跃了讨论气氛。 Rainer Weiss:详细解释了引力波的物理本质,即时空的涟漪,以及探测引力波的原理和方法。他回顾了LIGO项目的漫长发展历程,包括早期遇到的资金困难、技术挑战以及对黑洞存在的质疑。他还分享了2015年9月14日探测到引力波信号时的激动心情,以及对未来引力波研究的展望。 Janna Levin:引导讨论,提出问题,并与Rainer Weiss进行深入探讨,例如引力波对物理环境的影响、引力波的来源、LIGO探测器的建造过程以及引力波探测的意义。她还表达了对Rainer Weiss工作的敬佩之情。 Matt Kirshen:参与讨论,提出一些公众关心的问题,例如引力波是否能帮助时间旅行、引力波对人类的影响以及引力波的特性。 Rainer Weiss:详细解释了引力波的物理本质,并用通俗易懂的方式解释了复杂的科学概念。他分享了LIGO项目的发展历程,以及在探测引力波过程中遇到的挑战和突破。他还回答了关于引力波速度、双缝实验以及引力波与其他物理现象相互作用等问题。

Deep Dive

Key Insights

Why did the discovery of gravitational waves cause such a huge public reaction?

The discovery of gravitational waves caused a significant public reaction because it was a groundbreaking confirmation of Einstein's theory of general relativity, opening a new window into the universe. The announcement was so impactful that it halted daily activities, capturing global attention and excitement.

Why are gravitational waves described as a distortion of space and time?

Gravitational waves are described as a distortion of space and time because they are ripples in the fabric of spacetime caused by the acceleration of massive objects. These waves stretch and compress space in a perpendicular direction to their motion, and the effect is measured as a change in distance between objects.

Why did Rainer Weiss face skepticism when he first proposed building LIGO?

Rainer Weiss faced skepticism when he first proposed building LIGO because the concept of measuring an incredibly small effect, a strain of 10 to the minus 21, seemed practically impossible. Additionally, there was doubt about the existence of black holes, which were expected to be the primary sources of gravitational waves.

Why are gravitational waves so hard to detect?

Gravitational waves are hard to detect because they cause extremely tiny distortions in space-time, on the order of a millionth of a trillionth of a meter. The strain is 10 to the minus 21, and the effect is so subtle that it requires highly sensitive instruments like LIGO to measure it.

Why did Einstein initially doubt the physical significance of gravitational waves?

Einstein initially doubted the physical significance of gravitational waves because his calculations suggested that the energy and forces required to produce detectable waves were so immense that it would be practically impossible. He believed that the waves would not have any measurable physical consequences.

Why is the first detection of gravitational waves by LIGO considered a major milestone in astrophysics?

The first detection of gravitational waves by LIGO is considered a major milestone because it confirmed a key prediction of Einstein's theory of general relativity and opened a new way to observe the universe. This detection provided direct evidence of black hole collisions and allowed scientists to study phenomena that are invisible to traditional telescopes.

Why can't gravitational waves be used for time travel?

Gravitational waves cannot be used for time travel because they do not have the capability to manipulate time in a way that would allow for backward or forward travel. While they can stretch and compress space, they do not affect the flow of time in a manner that would enable time travel.

Why are LIGO's mirrors displaced by such a small amount?

LIGO's mirrors are displaced by an extremely small amount, about 10 to the minus 18 meters, because the strain of gravitational waves is incredibly small, around 10 to the minus 21. The mirrors are part of a highly sensitive interferometer designed to detect these minute changes in distance over a four-kilometer baseline.

Why did the first gravitational wave detection only last a quarter of a second?

The first gravitational wave detection lasted only a quarter of a second because the two black holes were only in LIGO's sensitive frequency band during the final moments of their collision. As they spiraled closer, the frequency of the waves increased, and LIGO was only able to detect the waves once they entered its operational range.

Shownotes Transcript

What is a gravitational wave? Janna Levin and comedian Matt Kirshen sit down with physicist Rainer Weiss to discuss LIGO, black holes, and the physics of gravitational waves. 

(Originally Aired October 4, 2016)

NOTE: StarTalk+ Patrons can listen to this entire episode commercial-free here: https://startalkmedia.com/show/deciphering-gravitational-waves-janna-levin-startalk-stars/)

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