Category: SCIENCE

  • Is fundamental science a victim of its own success?

    Is fundamental science a victim of its own success?

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    Some think the reason fundamental scientific revolutions are so rare is because of groupthink. It’s not; it’s hard to mess with success.

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  • Ask Ethan: Will the Universe ever reach equilibrium?

    Ask Ethan: Will the Universe ever reach equilibrium?

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    The expanding Universe, in many ways, is the ultimate out-of-equilibrium system. After enough time passes, will we eventually get there?

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  • The ultimate fate of every star that’s ever lived

    The ultimate fate of every star that’s ever lived

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    In ~7 billion years, our Sun will run out of fuel and die. So will every star, eventually. Here are the different fates they’ll encounter.

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  • Why reimagining the particle accelerator is so challenging

    Why reimagining the particle accelerator is so challenging

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    CERN’s Large Hadron Collider is the most powerful particle accelerator ever. To go even further, we’ll have to overcome something big.

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  • The compelling case for axions as our dark matter | by Ethan Siegel | Starts With A Bang! | Apr, 2024

    The compelling case for axions as our dark matter | by Ethan Siegel | Starts With A Bang! | Apr, 2024

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    Axions, one of the leading candidates for dark matter, may be able to be converted to photons (and vice versa) under the right conditions. If we can cause and control their conversion, we might discover our first particle beyond the Standard Model, and possibly solve the dark matter and strong CP problems as well. This would imply that we do live in a Universe with strong CP-violation, but only a tiny amount of it: below the experimental and observational thresholds. (Credit: Sandbox Studio, Chicago, Symmetry Magazine/Fermilab and SLAC)

    The majority of the matter in our Universe isn’t made of any of the particles in the Standard Model. Could the axion save the day?

    Astrophysically, normal matter — even with all the different forms it can take — cannot on its own explain the Universe we observe. Beyond all the stars, planets, gas, dust, plasma, black holes, neutrinos, photons, and more, there’s an overwhelming suite of evidence suggesting that the Universe contains two ingredients whose origins remain unknown: dark matter and dark energy. Dark matter, in particular, has an incredible amount of astrophysical evidence supporting its existence and abundance — outmassing normal matter by a 5:1 ratio. Still, its particle nature remains elusive, though we’re quite certain it must have been cold, or slow-moving at early times, rather than hot, where it would have moved faster in the young Universe.

    One of the leading candidates for its nature, the axion, remains compelling more than 40 years after it was first hypothesized, though it’s rarely even presented to the general public. Could this intriguing theoretical particle be the solution to the dark matter puzzle? That’s what Reggie Grünenberg wants to know, asking:

    “Axions are speculative particles and hot candidates for dark matter particles that are supposed to have been created primarily in the Big Bang and since then permanently within the cores of stars through a mechanism called the Primakoff effect. This would mean that stars would ‘produce’ dark matter — and that they would need to lose this way much more mass than through nuclear fusion. And that the amount of dark matter in galaxies would grow over time, thus accelerating orbiting stars ever more. Could this model really work?”

    There’s a lot to unpack here. But if we go one step at a time, you just might come away thinking that the axion could one day be the solution to the greatest cosmic mystery of all.

    The particles and antiparticles of the Standard Model have now all been directly detected, with the last holdout, the Higgs boson, falling at the LHC earlier this decade. Today, only the gluons and photons are massless; everything else has a non-zero rest mass. (Credit: E. Siegel/Beyond the Galaxy)

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  • Starts With A Bang podcast #104 — The magnetized galactic center

    Starts With A Bang podcast #104 — The magnetized galactic center

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    The center of the galaxy doesn’t just host stars and a black hole, but an enormous set of rich gassy and dusty features. Find out more!

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  • What was it like when mammals appeared and thrived? | by Ethan Siegel | Starts With A Bang! | Apr, 2024

    What was it like when mammals appeared and thrived? | by Ethan Siegel | Starts With A Bang! | Apr, 2024

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    During the Cambrian explosion, some 550–600 million years ago, the first complex, differentiated, macroscopic, multicellular, sexually-reproducing animals came to dominate the oceans. Over the next half a billion years, evolution would take life in many different directions. By the time the asteroid eliminating the dinosaurs arrived, 65 million years ago, mammals had diversified in a number of directions, with the earliest primates splitting off just before that great event. Modern lemurs, shown here, likely bear a strong resemblance to those early primates. (Credit: Bas Czerwinski/AFP/Getty Images)

    Although mammals may be the dominant form of life today, we’re relative newcomers on planet Earth. Here’s our place in natural history.

    The evolution of life on our planet didn’t take an inevitable course to bring human beings about, but rather appears to have led to us through a series of remarkable but not necessarily mandatory events. When planet Earth first formed, all the raw ingredients for life to emerge — atoms, molecules, a potentially habitable planet at the right distance from its star — were serendipitously in place. While life itself arose relatively quickly (within the first few hundred million years) on Earth, it took billions of years for that life to become complex, differentiated, and macroscopic. The four key developments that took us there were:

    • horizontal gene transfer, enabling an organism to gain useful genetic sequences from other species,
    • eukaryotic cells, whereby individual cells come to possess their own specialized organelles, enabling the performance of unique functions,
    • multicellularity, allowing further specialization and differentiation,
    • and sexual reproduction, enabling slowly-reproducing organisms to have dramatically different DNA…

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  • Ask Ethan: How do symmetries lead to conservation laws?

    Ask Ethan: How do symmetries lead to conservation laws?

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    First derived by Emmy Noether, for every symmetry a theory possesses, there’s an associated conserved quantity. Here’s the profound link.

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  • Particle physics finally charts a healthy path forward | by Ethan Siegel | Starts With A Bang! | Apr, 2024

    Particle physics finally charts a healthy path forward | by Ethan Siegel | Starts With A Bang! | Apr, 2024

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    On the right, the gauge bosons, which mediate the three fundamental quantum forces of our Universe, are illustrated. There is only one photon to mediate the electromagnetic force, there are three bosons mediating the weak force, and eight mediating the strong force. This suggests that the Standard Model is a combination of three groups: U(1), SU(2), and SU(3), whose interactions and particles combine to make up everything known in existence. Despite the success of this picture, many puzzles still remain. (Credit: Daniel Domingues/CERN)

    A great many cosmic puzzles still remain unsolved. By embracing a broad and varied approach, particle physics heads toward a bright future.

    Just a decade ago, the field of particle physics looked to be in a state of chaos. The Large Hadron Collider had recently turned on, and although they found the Higgs boson — the final undiscovered particle predicted by the Standard Model — it failed to turn up any evidence for any of the other leading theories that would take us beyond the Standard Model. Fermilab, the prior leader in the energy frontier, shut down its main accelerator permanently, and puzzles such as:

    • the origin of neutrino mass,
    • the nature of dark matter,
    • and the origin of the matter-antimatter asymmetry,

    seemed to be stagnating, with little progress to show on either the experimental or theoretical fronts.

    Moreover, particle physicists themselves seemed to be bickering and in disarray as to what they should do next. Would there be enough value to justify a new, more powerful accelerator than the Large Hadron Collider? How should we be probing the behavior of neutrinos in order to understand neutrino mass? Are we taking…

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  • 5 total mistakes to avoid at the April 8, 2024 solar eclipse | by Ethan Siegel | Starts With A Bang! | Apr, 2024

    5 total mistakes to avoid at the April 8, 2024 solar eclipse | by Ethan Siegel | Starts With A Bang! | Apr, 2024

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    This image, of the Sun’s inner corona and prominences on the Sun, was taken during the April 20, 2023 total solar eclipse. Exquisite views of what’s occurring just off of the Sun’s disk are best captured during a total solar eclipse. (Credit: Phil Hart)

    There are only a precious few minutes of totality during even the best solar eclipses. Don’t waste yours making these avoidable mistakes.

    On April 8, 2024, millions of North Americans will enjoy a spectacular total solar eclipse.

    The path of totality of the April 8, 2024 total solar eclipse cuts from southwest Mexico up through Texas, Oklahoma, Arkansas, Missouri, Illinois, Indiana, Ohio, Pennsylvania, New York, Vermont, New Hampshire, Maine, and Canada. Everyone along the center-line of the eclipse in 2024 also experienced at least a partial eclipse on October 14, 2023, and a penumbral lunar eclipse on March 25, 2024. (Credit: Great American Eclipse, LLC)

    For up to 4 minutes and 30 seconds, the Moon’s shadow will bring darkness to the daytime.

    This photograph from the International Space Station shows the shadow of the Moon falling on the Earth during a total solar eclipse. Although the Moon’s shadow passes rapidly over the surface of the Earth, the International Space Station moves more than twice as rapidly. (Credit: International Space Station/Reuters)

    Avoid these five common mistakes to make the most of your experience.

    This photograph, taken during the 2017 total solar eclipse, shows the Sun being eclipsed by the Moon during totality. Note how, although the sky is darkened closest to the Sun, the horizon is still illuminated by direct sunlight. The closer you are to the center-line of totality and the longer the duration of the eclipse, the darker the overall sky becomes, allowing observers to see fainter, dimmer objects. You will miss details such as this if you spend all of totality’s time attempting to photograph the eclipse. (Credit: Joe Sexton/Jesse Angle)

    1.) Don’t spend much time worrying about photography.

    This photograph of the eclipsed Sun during totality shows the asymmetric corona and the last remnant of a tiny bit of sunlight poking through a crater on the Moon: one of Baily’s beads. (Credit: Ricardo Garza-Grande)

    Totality is brief, and eclipse photography is very finicky.

    The solar corona, as shown here, is imaged out to 25 solar radii during the 2006 total solar eclipse. The longer the duration of a total solar eclipse, the darker the sky becomes and the better the corona and background astronomical objects can be seen. Experienced, serious eclipse photographers can construct images such as these from their eclipse data. (Credit: Martin Antoš, Hana Druckmüllerová, Miloslav Druckmüller)

    Professional eclipse photographers will produce outstanding photographs, but every individual can enjoy a first-person experience.

    Although your unaided eye may be of use in spying details in the solar corona, only long-exposure eclipse photography, done at a professional level, can bring out details such as those exposed here in the inner corona during the 2009 solar eclipse. (Credit: Miloslav Druckmüller, Peter Aniol)

    2.) Don’t leave your eclipse glasses on during totality.

    Either eclipse glasses, solar filters, or welder’s shades (that are at least shade 14 or darker) are all tools that humans can leverage to view the Sun directly during a partial or annular solar eclipse, or even during no eclipse at all. During totality, however, you must remove them, or you won’t see anything at all. (Credit: GPA Photo Archive)

    Once the Sun goes completely dark through your eclipse glasses, remove them.

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