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NASA’s James Webb Space Telescope (JWST) recently used its powerful Near-Infrared Camera (NIRCam) to peer into the very center of our Milky Way Galaxy, revealing stunning details in a star-forming region known as Sagittarius C (Sgr C) like never before, which includes approximately 500,000 in this single image. Sgr C is located approximately 300 light-years from the exact center of the Milky Way known as Sagittarius A*, which is a supermassive black hole. For context, the Milky Way is approximately 105,000 light-years across, so Sgr C being only 300 light-years from the center of the Milky Way is extremely close.

“The galactic center is a crowded, tumultuous place. There are turbulent, magnetized gas clouds that are forming stars, which then impact the surrounding gas with their outflowing winds, jets, and radiation,” said Dr. Rubén Fedriani, who is a Juan de la Cierva Postdoctoral Fellow at the Instituto Astrofísica de Andalucía in Spain and a co-investigator of the project. “Webb has provided us with a ton of data on this extreme environment, and we are just starting to dig into it.”

With a gravitational field so strong that not even light can escape its grip, black holes are probably the most interesting and bizarre objects in the universe.

Due to their extreme properties, a theoretical description of these celestial bodies is impossible within the framework of Newton’s classical theory of gravity. It requires the use of general relativity, the theory proposed by Einstein in 1915, which treats gravitational fields as deformations in the fabric of space-time.

Black holes are usually formed from the collapse of massive stars during their final stage of evolution. Therefore, when a black hole is born, its mass does not exceed a few dozen solar masses.

In this video, we will explain a new paper that suggests that there was a second big bang, or a “Dark Big Bang”, that created different kinds of dark matter particles, some of which could be very massive. We will explain how this hypothesis could solve two of the biggest mysteries in cosmology: the origin of the universe and the nature of dark matter. We will also explain how this hypothesis could be tested by future experiments, such as gravitational wave detectors and gamma-ray telescopes. The paper offers a new perspective on the history and structure of the universe, and challenges some of the assumptions and predictions of the standard cosmological model. The paper also opens new possibilities for exploring and understanding the dark sector of the universe, which could reveal new physics and phenomena. So, stay tuned and get ready to explore the dark side of the big bang.

Chapters:
00:00 Introduction.
02:00 The Dark Big Bang.
03:55 The Origin of the Universe.
06:22 The Nature of Dark Matter.
08:27 Outro.
09:03 Enjoy.

Continue reading “Two Big Bangs, One Universe: A New Study That Challenges the Standard Cosmological Model” »

An innovative experiment flying aboard NASA’s Psyche mission just hit its first major milestone by successfully carrying out the most distant demonstration of laser communications. The tech demo could one day help NASA missions probe deeper into space and uncover more discoveries about the origin of the universe.

Launched in mid-October, Psyche is currently en route to catch humanity’s first glimpse of a metal asteroid between the orbits of Mars and Jupiter. The spacecraft will spend the next six years traveling about 2.2 billion miles (3.6 billion kilometers) to reach its namesake, located in the outer part of the main asteroid belt.

Along for the ride is the Deep Space Optical Communications technology demonstration, or DSOC, which is carrying out a mission of its own during the first two years of the journey.

A groundbreaking study by University of Leeds scientists proposes that Be stars are part of triple star systems, not binary systems as previously thought. This finding, derived from Gaia satellite data, challenges conventional star formation theories and could impact our knowledge of black holes, neutron stars, and gravitational waves.

Gravitational waves are distortions or ripples in the fabric of space and time. They were first detected in 2015 by the Advanced LIGO detectors and are produced by catastrophic events such as colliding black holes, supernovae, or merging neutron stars.

Observations from the Event Horizon Telescope show that the supermassive black hole at the heart of the galaxy M87 has twisted magnetic fields that help matter and light escape from the immense gravit.

Sean Carroll speaking at the 6th International FQXi Conference, “Mind Matters: Intelligence and Agency in the Physical World.”

The Foundational Questions Institute (FQXi) catalyzes, supports, and disseminates research on questions at the foundations of physics and cosmology, particularly new frontiers and innovative ideas integral to a deep understanding of reality but unlikely to be supported by conventional funding sources.

Continue reading “Sean Carroll on Causality and the Arrow of Time” »

Join Brian Greene and Juan Maldacena as they explore a wealth of developments connecting black holes, string theory, quantum gravity, quantum entanglement, wormholes, and the holographic principle.

This program is part of the Big Ideas Series, made possible with support from the John Templeton Foundation.

Continue reading “String Theory, Quantum Gravity and Black Holes (Or, Are We Holograms?)” »

The supermassive black hole at the heart of our galaxy isn’t just spinning — it’s doing so at almost maximum speed, dragging anything near it along for the ride.

Physicists calculated the rotational speed of the Milky Way’s supermassive black hole, called Sagittarius A* (Sgr A•, by using NASA’s Chandra X-ray Observatory to view the X-rays and radio waves emanating from outflows of material.