Lifeboat Foundation: Safeguarding Humanity
Toggle light / dark theme

Blog

Category: physics

A University of Toronto astronomer’s research suggests the solar system is surrounded by a magnetic tunnel that can be seen in radio waves.

Jennifer West, a research associate at the Dunlap Institute for Astronomy & Astrophysics, is making a scientific case that two bright structures seen on opposite sides of the sky – previously considered to be separate – are actually connected and are made of rope-like filaments. The connection forms what looks like a tunnel around our solar system.

The data results of West’s research have been published in the Astrophysical Journal.

Read more | >

For the first time, physicists have been able to directly measure one of the ways exploding stars forge the heaviest elements in the Universe.

By probing an accelerated beam of radioactive ions, a team led by physicist Gavin Lotay of the University of Surrey in the UK observed the proton-capture process thought to occur in core-collapse supernovae.

Not only have scientists now seen how this happens in detail, the measurements are allowing us to better understand the production and abundances of mysterious isotopes called p-nuclei.

Read more | >

Is there anything out there?

The concept of primordial black holes has waxed and waned in scientific circles over the decades. At first, it was a fascinating possibility. After all, the first few seconds of the big bang were pretty heady times, and there may have been large enough differences in density to generate black holes of all sorts of sizes, from microscopic to gigantic. But repeated observations have continually been unable to come up with any conclusive evidence for their existence.

And then there’s dark matter, the mysterious substance that makes up the vast bulk of matter in the cosmos. Scientists aren’t exactly sure what lies behind dark matter, and primordial black holes are a tantalizing possibility.

But if the universe is flooded with innumerable small black holes, eventually some of those black holes will find each other and merge. And our gravitational wave observatories should be sensitive enough to detect the resulting ripples in spacetime.

Read more | >

Low-frequency gravitational waves could unlock the secrets of the ancient universe.

But scientists still can’t detect these waves at low frequencies that are often the result of even more massive objects colliding with one another or events that took place shortly after the Big Bang.

A team of researchers from the University of Birmingham suggests combining different methods to detect ultra low-frequency gravitational waves that hold the mystery of ancient black holes and the early universe.

Read more | >

Is Planetary Defense PI in the Sky?

In February of 2,013 skywatchers around the world turned their attention toward asteroid 2012 DA14, a cosmic rock about 150 feet (50 meters) in diameter that was going to fly closer to Earth than the spacecraft that bring us satellite TV.

Little did they realize as they prepared for the once-in-several-decades event that another bit of celestial debris was hurtling toward Earth, with a more direct heading. On February 15 2013, the Chelyabinsk meteor, a roughly 62-foot (19 meter)-diameter asteroid exploded over the city of Chelyabinsk, Russia, as it entered Earth’s atmosphere at a shallow angle. The blast shattered windows and damaged buildings, and nearly two thousand people were hurt, though thankfully no one died.

Read more | >

An international team of researchers has made the world’s most precise measurement of the neutron’s lifetime, which may help answer questions about the early universe.

An international team of physicists led by researchers at Indiana University Bloomington has announced the world’s most precise measurement of the neutron’s lifetime.

The results from the team, which encompasses scientists from over 10 national labs and universities in the United States and abroad, represent a more than two-fold improvement over previous measurements — with an uncertainty of less than one-tenth of a percent.

Read more | >

A new study showing how the explosion of a stripped massive star in a supernova can lead to the formation of a heavy neutron star or a light black hole resolves one of the most challenging puzzles to emerge from the detection of neutron star mergers by the gravitational wave observatories LIGO and Virgo.

The first detection of gravitational waves by the Advanced Laser Interferometer Gravitational-Wave Observatory (LIGO) in 2017 was a star merger that mostly conformed to the expectations of astrophysicists. But the second detection, in 2,019 was a merger of two whose combined mass was unexpectedly large.

“It was so shocking that we had to start thinking about how to create a heavy neutron star without making it a pulsar,” said Enrico Ramirez-Ruiz, professor of astronomy and astrophysics at UC Santa Cruz.

Read more | >