How do supermassive black holes get super massive?

2024-09-09

UNIVERSITY PARK, Pa. — By combining forefront X-ray observations with state-of-the-art supercomputer simulations of the buildup of galaxies over cosmic history, researchers have provided the best modeling to date of the growth of the supermassive black holes found in the centers of galaxies. Using this hybrid approach, a research team led by Penn State astronomers derived a complete picture of black-hole growth over 12 billion years, from the Universe’s infancy at around 1.8 billion years old to now at 13.8 billion years old.

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First flight of HELIX

2024-07-10

The High Energy Light Isotope eXperiment is designed to measure various isotopes of cosmic ray nuclei, which are sensitive to the history of propagation of these energetic particles through our Milky Way galaxy, and which are linked to energetic interactions in the interstellar medium (yielding antimatter as well as rare nuclei). The instrument had its first stratospheric balloon flight on May 28, 2024 from the Esrange rocket/balloon base in northern Sweden, landing on Ellesmere Island in the Canadian high Arctic after more than 6 days. The Penn State group includes IGC faculty Stephane Coutu and Isaac Mognet, and past and present students Heather Allen, Carl Chen, Alex Pazoki and Monong Yu.

2024-06-18

When stars collapse, they can leave behind incredibly dense but relatively small and cold remnants called neutron stars. If two stars collapse in close proximity, the leftover binary neutron stars spiral in and eventually collide, and the interface where the two stars begin merging becomes incredibly hot. New simulations of these events show hot neutrinos — tiny, essentially massless particles that rarely interact with other matter — that are created during the collision can be briefly trapped at these interfaces and remain out of equilibrium with the cold cores of the merging stars for 2 to 3 milliseconds. During this time, the simulations show that the neutrinos can weakly interact with the matter of the stars, helping to drive the particles back toward equilibrium — and lending new insight into the physics of these powerful events.

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2024-06-11

A team of astronomers, including Penn State researchers, from the Sloan Digital Sky Survey (SDSS) has used eight years of monitoring observations to discover unexpected changes in the winds surrounding a distant black hole.

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2024-06-11

A team of astronomers, including Penn State researchers, from the Sloan Digital Sky Survey (SDSS) has used eight years of monitoring observations to discover unexpected changes in the winds surrounding a distant black hole.

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2024-03-21

Astronomers have revealed that a brilliant supermassive black hole is not living up to expectations. Although it is responsible for high levels of radiation and powerful jets, this giant black hole is not as influential on its surroundings as many of its counterparts in other galaxies. A team including IGC faculty W. Niel Brandt, the Eberly Family Chair Professor of Astronomy and Astrophysics and professor of physics at Penn State, recently published this study in the Monthly Notices of the Royal Astronomical Society.

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2024-03-12

The IceCube Neutrino Observatory, a cubic-kilometer-sized neutrino telescope at the South Pole, has observed a new kind of astrophysical messenger. In a new study recently accepted for publication as an Editors' Suggestion by the journal Physical Review Letters and available online as a preprint, the IceCube collaboration, including Penn State researchers, presented the discovery of seven of the once-elusive astrophysical tau neutrinos.

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