Lifeboat Foundation

Google on Monday announced Willow, its latest, greatest quantum computing chip. The speed and reliability performance claims Google’s made about this chip were newsworthy in themselves, but what really caught the tech industry’s attention was an even wilder claim tucked into the blog post about the chip.

Google Quantum AI founder Hartmut Neven wrote in his blog post that this chip was so mind-boggling fast that it must have borrowed computational power from other universes.

Ergo the chip’s performance indicates that parallel universes exist and “we live in a multiverse.”

For centuries, gravity has been one of the most captivating and puzzling forces in the universe. Thanks to the groundbreaking work of Isaac Newton and Albert Einstein, we have a robust understanding of how gravity governs the behavior of planets, stars, and even galaxies. Yet, when we look at extreme scenarios, such as the intense gravitational fields near black holes or the mysterious quantum world, our understanding starts to break down. New research and theories, however, suggest that the key to solving these mysteries may finally be within reach.

In our daily lives, gravity is a constant presence. It’s what keeps us grounded to the Earth, dictates the orbits of planets, and ensures that satellites stay in orbit around our planet. Thanks to Einstein’s general theory of relativity, scientists have been able to make highly accurate predictions about the movement of celestial bodies, calculate tides, and even send probes to the farthest reaches of the solar system.

Yet, when gravity’s effects become more extreme—such as inside black holes or during the birth of the universe—it becomes much more difficult to model. Similarly, when we turn our attention to the quantum realm of subatomic particles, Einstein’s theory breaks down. To understand phenomena like the Big Bang or the inner workings of black holes, physicists have long known that we need a new, unified theory of gravity.

Black holes have long fascinated scientists, known for their ability to trap anything that crosses their event horizon. But what if there were a counterpart to black holes? Enter the white hole—a theoretical singularity where nothing can enter, but energy and matter are expelled with immense force.

First proposed in the 1970s, white holes are essentially black holes in reverse. They rely on the same equations of general relativity but with time flowing in the opposite direction. While a black hole pulls matter in and lets nothing escape, a white hole would repel matter, releasing high-energy radiation and light.

Despite their intriguing properties, white holes face significant scientific challenges. The laws of thermodynamics, particularly entropy, make it improbable for matter to move backward in time, as white holes would require. Additionally, introducing a singularity into the Universe without a preceding collapse defies current understanding of cosmic evolution.

The Bubble Universe: A Bold New Theory

Researchers at Uppsala University in Sweden have introduced a revolutionary theory suggesting that our Universe exists as a four-dimensional bubble within a higher-dimensional space. This bubble concept is part of an attempt to unravel the mystery of dark energy, the enigmatic force causing the Universe’s rapid expansion.

With the imaging spectrograph blocking out the bright light from the region at the heart of the quasar, Hubble was able to see the structure around the black hole like never before.

Bin Ren of the Côte d’Azur Observatory and Université Côte d’Azur in France explained in a NASA statement that Hubble found lots of “weird things” around the feeding supermassive black hole powering 3C 273.

“We’ve got a few blobs of different sizes and a mysterious L-shaped filamentary structure,” Ren said. “This is all within 16,000 light-years of the black hole.”

Even matter ejected by black holes can run into objects in the dark. Using NASA’s Chandra X-ray Observatory, astronomers have found an unusual mark from a giant black hole’s powerful jet striking an unidentified object in its path.

The discovery was made in a galaxy called Centaurus A (Cen A), located about 12 million light-years from Earth. Astronomers have long studied Cen A because it has a supermassive black hole in its center sending out spectacular jets that stretch out across the entire galaxy. The black hole launches this jet of high-energy particles not from inside the black hole, but from intense gravitational and magnetic fields around it.

Continue reading “Chandra sees black hole jet stumble into something in the dark” »

Ultra-high energy cosmic rays, which emerge in extreme astrophysical environments—like the roiling environments near black holes and neutron stars—have far more energy than the energetic particles that emerge from our sun. In fact, the particles that make up these streams of energy have around 10 million times the energy of particles accelerated in the most extreme particle environment on earth, the human-made Large Hadron Collider.

Where does all that energy come from? For many years, scientists believed it came from shocks that occur in extreme astrophysical environments—when, for example, a star explodes before forming a black hole, causing a huge explosion that kicks up particles.

That theory was plausible, but, according to new research published in The Astrophysical Journal Letters, the observations are better explained by a different mechanism. The source of the cosmic rays’ energy, the researchers found, is more likely magnetic turbulence. The paper’s authors found that magnetic fields in these environments tangle and turn, rapidly accelerating particles and sharply increasing their energy up to an abrupt cutoff.

New analysis supports Einstein’s relativity and narrows neutrino mass ranges, hinting at evolving dark energy.

Gravity, the fundamental force sculpting the universe, has shaped tiny variations in matter from the early cosmos into the vast networks of galaxies we see today. Using data from the Dark Energy Spectroscopic Instrument (DESI), scientists have traced the evolution of these cosmic structures over the past 11 billion years. This research represents the most precise large-scale test of gravity ever conducted, offering unprecedented insights into the universe’s formation and behavior.

Introduction to DESI and its global impact.

Researchers have developed a new computational method to explore the neutron matter inside neutron stars at densities higher than previously studied.

This method provides insights into the behavior of neutrinos during supernova explosions, enhancing the accuracy of simulations and potentially improving our understanding of such cosmic events.

Advances in Neutron Matter Simulation.