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Part 3: Extended Physics Analyses with the DESI DR2 BAO

Part 3: Extended Physics Analyses with the DESI DR2 BAO

by Jessie Thwaites, Sarah Stevenson | Oct 6, 2025 | Daily Paper Summaries, PRJ

Today Astrobites is featuring results from the DESI DR2, published today in PRJ! In Part 3, we discuss 2 additional papers using the BAO measurement to perform additional analyses.

Part 1: Key Results from the DESI DR2

Part 1: Key Results from the DESI DR2

by Sarah Stevenson, Sumeet Kulkarni | Oct 6, 2025 | Daily Paper Summaries, PRJ

Today Astrobites is featuring results from the DESI DR2, published today in PRJ! In Part 1, we cover the key results papers describing their measurements with DR2.

Using Galaxy Halos to Study Baryonic Feedback in FLAMINGO

Using Galaxy Halos to Study Baryonic Feedback in FLAMINGO

by Lindsey Gordon | Oct 4, 2025 | Daily Paper Summaries, PRJ

Today’s authors use FLAMINGO simulations to probe the tension between different observational methods of estimating cosmological parameters.

If primordial black holes are dark matter, would we know?

If primordial black holes are dark matter, would we know?

by Annelia Anderson | Sep 8, 2025 | Daily Paper Summaries

Today’s paper explores the detectability of primordial black holes as a potential dark matter candidate.

The Continuing Saga of the Not-So-Constant Constant.

The Continuing Saga of the Not-So-Constant Constant.

by William Smith | Aug 30, 2025 | Daily Paper Summaries, PRJ

The cosmological constant is a constant, right? The word “constant” is right there in the name for goodness sakes. But growing evidence suggests this might not be the case after all. Today’s authors further investigate the DESI analysis pushing our understanding of dark energy.

Using Large-scale structures and gravitational wave sources to measure the expansion rate

Using Large-scale structures and gravitational wave sources to measure the expansion rate

by Abbé Whitford | Jul 17, 2025 | Daily Paper Summaries

In today’s astrobite we explore a new approach that has been developed to measure the Universal expansion rate, involving gravitational waves from merging black holes and the large-scale structure of the Universe.

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