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Using Gravitational Waves to Measure the Expansion of the Universe

2. Finding the Expansion Rate of the Universe

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About this Lecture

Lecture

In the second mini-lecture, we take a step back to recall the work done by Edwin Hubble. In particular, we focus on: (i) Hubble’s work with pulsating stars known as cepheid variable stars (an extension of the work done by Henrietta Leavitt), which allowed him to deduce the distances from Earth of these stars and nearby stars; (ii) how we can use the redshift or blueshift of spectral lines of light observed from distant objects to determine the speed and direction these objects are moving; (iii) Hubble’s use of cepheid variable stars and redshift, which allowed him to conclude that the Universe is expanding and led to the Hubble Law (Hubble-Lemaître Law) and the Big Bang Theory; (iv) the Hubble Space Telescope, which sought to refine Hubble’s findings; (v) the speeding up of the expansion rate of the Universe, which we believe to be caused by Dark Energy; and (vi) the cosmic microwave background (CMB), which helped us extrapolate the current expansion rate of the Universe, but which does not give us the same result as the cepheid variable star approach!

Course

In this course, Professor Martin Hendry (University of Glasgow) discusses how we can use gravitational wave detections to help us refine our measurement of the expansion rate of the Universe. In the first mini-lecture, we introduce gravitational waves, first as a prediction made by Einstein in his theory of gravity and then as an observation made nearly 100 years later with the LIGO interferometer detectors. In the second mini-lecture, we discuss Edwin Hubble’s work that led to the discovery of the expansion of the Universe and how his work has been extended in more recent times. In the third mini-lecture, we discuss how gravitational waves can be used to help us find the expansion rate of the Universe, and in the fourth mini-lecture, we look at a specific event, GW 170817, that allowed us to make the first measurement of the Universe’s expansion rate using gravitational waves. In the fifth mini-lecture, we consider some notable gravitational wave detections and what the future holds.

Lecturer

Martin Hendry is a Professor of Gravitational Astrophysics and Cosmology at the University of Glasgow. His primary research interests lie in gravitational wave astronomy, statistical methods for the analysis of astrophysical and cosmological data sets, and applications of gravitational lensing. He is a member of the LIGO Scientific Collaboration (LSC), which has been awarded the 2016 Special Breakthrough Prize for Fundamental Physics, the Physics World Breakthrough of the Year for 2016 and 2017, and the President's Medal of the Royal Society of Edinburgh. He serves as the chair of LSC Education and Public Outreach group and is the co-chair of the Advocacy and Outreach Group of the recently established International LISA Consortium. Professor Hendry is also an elected follow of the Royal Society of Edinburgh and a fellow of the Institute of Physics (IOP), serving as chair of the IOP in Scotland from 2015-2017. In 2010, he was invited by Learning and Teaching Scotland to join the Maths Excellence Group and Physics Qualifications Design Team for the Curriculum for Excellence, where he helped to redesign the high school physics curriculum in Scotland. He has won various awards in public outreach, including the Royal Society of Edinburgh’s Senior Prize for public engagement.

Cite this Lecture

APA style

Hendry, M. (2022, January 14). Using Gravitational Waves to Measure the Expansion of the Universe - Finding the Expansion Rate of the Universe [Video]. MASSOLIT. https://massolit.io/courses/using-gravitational-waves-to-measure-the-expansion-of-the-universe/finding-the-expansion-rate-of-the-universe

MLA style

Hendry, Martin. "Using Gravitational Waves to Measure the Expansion of the Universe – Finding the Expansion Rate of the Universe." MASSOLIT, uploaded by MASSOLIT, 14 Jan 2022, https://massolit.io/courses/using-gravitational-waves-to-measure-the-expansion-of-the-universe/finding-the-expansion-rate-of-the-universe

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