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Continued analysis on the continuous search for continuous waves (continued)

Continued analysis on the continuous search for continuous waves (continued)

by William Lamb | Oct 12, 2023 | Daily Paper Summaries

Post-detection of a gravitational wave background, pulsar timing arrays could detect individual sources of gravitational waves, called Continuous Waves. Let’s find out what properties we expect them to have!

Can we identify the host galaxies of LISA sources?

Can we identify the host galaxies of LISA sources?

by William Lamb | Sep 19, 2023 | Daily Paper Summaries

The upcoming LISA mission promises to detect many gravitational wave events, but can it attribute any of them to a host galaxy? Let’s find out!

Both Pirouettes and Do-si-Dos: Why is there a bias in the black hole ballet?

Both Pirouettes and Do-si-Dos: Why is there a bias in the black hole ballet?

by Cole Meldorf | Sep 1, 2023 | Daily Paper Summaries

In this Astrobite, we look at black hole mergers in the accretion disks around supermassive black holes, because you can simply never have too many black holes!

Could the NANOGrav signal be primordial?

Could the NANOGrav signal be primordial?

by Emma Clarke | Aug 16, 2023 | Daily Paper Summaries

Pulsar timing array experiments recently reported evidence for a background of gravitational waves traveling through the universe. Is it possible that this signal is primordial in origin?

Vanishing Stars Surface New Island in the Massive Ocean

Vanishing Stars Surface New Island in the Massive Ocean

by Storm Colloms | Aug 12, 2023 | Daily Paper Summaries

In a magical act some stars could vanish from the night sky, today’s bite asks: can we can see them again as black holes?

How (and How Not) to Build High-Frequency Gravitational Wave Detectors

How (and How Not) to Build High-Frequency Gravitational Wave Detectors

by Emma Clarke | Aug 7, 2023 | Daily Paper Summaries

Detecting high-frequency gravitational waves is a challenging task. Today’s paper proposes several novel experimental methods with promising sensitivities.

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