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LISA Pathfinder: These magnetic results will attract your attention

LISA Pathfinder: These magnetic results will attract your attention

by Magnus L'Argent | Dec 21, 2024 | Daily Paper Summaries, PRJ

This organized magnetic noise is so fresh, so clean.

Red Giants Have it All: Dark Matter Constraints from Stellar Evolution

Red Giants Have it All: Dark Matter Constraints from Stellar Evolution

by Catherine Slaughter | Dec 7, 2024 | Daily Paper Summaries, PRJ

How can astronomers use existing understandings of stellar evolution to better study dark matter?

Cheat Sites & AI & Large Language Models, Oh My!

Cheat Sites & AI & Large Language Models, Oh My!

by Tori Bonidie | Dec 2, 2024 | Daily Paper Summaries, PRJ

The authors of today’s paper explore how students are using AI to aid them in their introductory physics course, how that usage impacts their scores, and how these students feel about the current landscape of AI as it pertains to their educational experiences.

Chasing Colliding Black Holes with Stellar Cluster Correlations

Chasing Colliding Black Holes with Stellar Cluster Correlations

by Storm Colloms | Nov 30, 2024 | Daily Paper Summaries, PRJ

Today’s astrobite looks at using mass and spin measurements of black hole binaries to learn about their formation in stellar clusters and beyond

A Galaxy Lost in the Gamma-Ray Sauce

A Galaxy Lost in the Gamma-Ray Sauce

by Delaney Dunne | Nov 16, 2024 | Daily Paper Summaries, PRJ

We’re still trying to understand what caused the emission seen in the Fermi Bubbles, massive lobes of gamma rays extending out of the Milky Way. Today’s authors argue that one of the Milky Way’s satellite galaxies is probably not an ingredient!

Looking on the bright side: gamma-ray predictions from supernova dark matter

Looking on the bright side: gamma-ray predictions from supernova dark matter

by Ivey Davis | Nov 9, 2024 | Daily Paper Summaries, PRJ

When we cannot measure particles directly, we have to look for their radiation byproducts. Today’s authors investigate the possibility of detecting dark matter being converted into gamma rays by the the most famous supernova’s remnant.

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