New data suggests universe may end in big crunch

Fresh analysis of dark energy observations indicates the universe could collapse in a big crunch after expanding for another 11 billion years. Cornell physicist Henry Tye's model, based on data from major surveys, predicts a total lifespan of about 33 billion years for the cosmos. This challenges long-held views of endless expansion.

The universe, currently aged 13.8 billion years and still expanding, faces a potential dramatic turnaround according to recent calculations. Henry Tye, the Horace White Professor of Physics Emeritus at Cornell University, has updated a model centered on the cosmological constant—a concept introduced by Albert Einstein over a century ago. His findings, detailed in the paper "The Lifespan of our Universe" published in the Journal of Cosmology and Astroparticle Physics, suggest the universe is approaching the midpoint of its existence, with a maximum expansion in roughly 11 billion years followed by contraction leading to a collapse in about 20 billion years.

Tye's conclusions draw from 2025 data releases by the Dark Energy Survey (DES) in Chile and the Dark Energy Spectroscopic Instrument (DESI) in Arizona. These observatories, which probe dark energy comprising 68% of the universe's mass and energy, show results that align closely despite their hemispheric separation. The data imply the cosmological constant may be negative, deviating from the positive value assumed for two decades that would sustain perpetual expansion.

"For the last 20 years, people believed that the cosmological constant is positive, and the universe will expand forever," Tye stated. "The new data seem to indicate that the cosmological constant is negative, and that the universe will end in a big crunch."

To reconcile the observations, Tye and co-authors Hoang Nhan Luu and Yu-Cheng Qiu propose a hypothetical low-mass particle that initially mimicked a constant but evolved over time, shifting the constant negative. "This big crunch defines the end of the universe," Tye wrote.

While the idea of a negative constant leading to collapse is not novel, Tye's model specifies the timeline. Further observations from projects like the Zwicky Transient Facility, the European Euclid space telescope, NASA's SPHEREx mission, and the Vera C. Rubin Observatory will test these predictions. Tye emphasizes the value in defining cosmic endpoints: "For our universe, it's also interesting to know, does it have a beginning? ... Does it have an end?"

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Researchers from the University of Illinois Urbana-Champaign and the University of Chicago have developed a novel approach to calculate the Hubble constant using gravitational waves from black hole collisions. This technique, known as the stochastic siren method, analyzes the background hum of faint mergers to potentially resolve the Hubble tension. The findings, accepted for publication in Physical Review Letters, offer improved precision with current data.

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Physicists at the University of Massachusetts Amherst propose that a record-breaking neutrino detected in 2023 originated from the explosion of a primordial black hole carrying a 'dark charge.' The particle's energy, 100,000 times greater than that produced by the Large Hadron Collider, puzzled scientists since only the KM3NeT experiment recorded it. Their model, published in Physical Review Letters, could also hint at the nature of dark matter.

Astronomers have produced the most detailed map of dark matter to date using NASA's James Webb Space Telescope, revealing how this invisible substance shaped the formation of galaxies and planets. The research, involving teams from Durham University, NASA's Jet Propulsion Laboratory, and Switzerland's École Polytechnique Fédéral de Lausanne, was published in Nature Astronomy. The map highlights dark matter's gravitational role in pulling ordinary matter together since the universe's early days.

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Astronomers using China's Einstein Probe telescope have observed a powerful X-ray flash that matches the predicted signature of a 'dirty fireball,' a theorized explosion from a dying massive star. The event, labeled EP241113a, originated from a galaxy about 9 billion light years away. This detection could reveal new details about how massive stars end their lives.

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