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James Webb just Found a Supernova That Could Break the Laws of Physics

In this episode, we explore how a triple-lens supernova observed by the James Webb Space Telescope could help solve the mystery of the Hubble tension, which is the discrepancy between different measurements of the expansion rate of the Universe. We also learn about the details of the supernova and the galaxy cluster that caused the gravitational lensing effect, and how JWST and other telescopes can use this supernova to test various cosmological models and parameters.

Paper Link:
https://arxiv.org/abs/2309.

Chapters:
00:00 Introduction.
01:10 How JWST Discovered a Rare and Triple-Lens Supernova.
04:13 How H0pe Can Measure the Expansion Rate in a New Way.
09:00 How hOpe can test various cosmological models.
11:26 Outro.
12:24 Enjoy.

Best Telescopes for beginners:
Celestron 70mm Travel Scope.
https://amzn.to/3jBi3yY

Celestron 114LCM Computerized Newtonian Telescope.
https://amzn.to/3VzNUgU

Celestron – StarSense Explorer LT 80AZ

Theoretical study shows that Kerr black holes could amplify new physics

Black holes are regions in space characterized by extremely strong gravity, which prevents all matter and electromagnetic waves from escaping it. These fascinating cosmic bodies have been the focus of countless research studies, yet their intricate physical nuances are yet to be fully uncovered.

Researchers at University of California–Santa Barbara, University of Warsaw and University of Cambridge recently carried out a theoretical study focusing on a class of known as extremal Kerr black holes, which are uncharged stationary black holes with a coinciding inner and outer horizon. Their paper, published in Physical Review Letters, shows that these black holes’ unique characteristics could make them ideal “amplifiers” of new, unknown .

“This research has its origin in a previous project started during my visit to UC Santa Barbara,” Maciej Kolanowski, one of the researchers who carried out the study, told Phys.org. “I started discussing very cold (so called, extremal) black holes with Gary Horowitz (UCSB) and Jorge Santos (at Cambridge). Soon we realized that in fact, generic extremal black holes look very different than it was previously believed.”

JWST’s first triple-image supernova could save the Universe

With future observations and as more time passes — both from new data and from data that’s still being analyzed and prepared by this collaboration — we may obtain the most precise and accurate measurement for the expansion rate of the Universe using the cosmic distance ladder method of all-time.

This triply-imaged supernova was not named “Supernova H0pe” in vain, as it really does give us hope that the answer to today’s greatest cosmic puzzle may indeed be written on the face of the Universe. With JWST going strong, we may have already found the galaxy cluster, and the gravitationally lensed system, that will resolve what’s been puzzling astronomers for the entirety of the 21st century.

Dark Photons Could Explain One of The Universe’s Greatest Mysteries

A shadowy form of light within a universe of hypothetical particles is getting some serious consideration as a means of discovering the identity of dark matter.

According to a comprehensive new analysis under quantum chromodynamics, the dark photon is a much better fit for the observed results of particle collider experiments than the standard model of particle physics, by quite a wide margin.

In fact, a team of researchers led by physicist Nicholas Hunt-Smith of the ARC Centre of Excellence for Dark Matter Particle Physics and the University of Adelaide in Australia calculated a confidence level of 6.5 sigma, suggesting the odds that dark photons don’t explain the observations are in the ballpark of one in a billion.

Scaled-Up Version Of Solar System Discovered Around Star That Will Go Supernova

Most exoplanets that have been discovered over the last few decades happened to go around stars that are roughly the same size as the Sun. Some are a bit bigger and many a lot smaller. Planets have been discovered around pulsars, the extreme end product of supernovae, so astronomers expect that planets are to be found around the massive star that will one day explode as a supernova. Two such planets have recently been discovered and the whole setup looks like a blown-up version of our own Solar System.

The star in question is called μ2 Sco which is part of the Scorpius-Centaurus association. This is a group of young stars, no older than 20 million years. Among them, μ2 Sco (pronounced Mew two, yes like the legendary Pokemon) is a massive, blue, hot star that weighs about nine times our Sun. The observations conducted in this study suggest the presence of two candidate companions.

These are called CC0 and μ2 Sco b. The first has not been confirmed completely yet. It appears to have a mass of about 18.5 times that of Jupiter. The team is confident in the detection of the second one, which has a mass of about 14.4 Jupiters, so it gets the proper planet name. The team uses the term planet.