A new simulation code from Perimeter Institute unlocks the hidden dynamics of self-interacting dark matter
Sandeep K S
Dec 1, 2025
1 min read
Updated: Dec 2, 2025
Introducing KISS-SIDM, a revolutionary code that bridges the gap in previous simulation methods by accurately modeling the critical intermediate-density range. This advancement not only accelerates and simplifies research, allowing it to be conducted on standard laptops, but also unveils new insights into galaxy evolution and black hole formation.
Scientists have uncovered the first robust evidence of a black hole and neutron star crashing together while orbiting in an oval path, challenging long-standing assumptions about cosmic pair formation.
Most neutron star-black hole pairs are expected to adopt circular orbits long before merging, their orbits slowly rounded out by the constant emission of gravitational waves over millions of years.
Far from the warmth of any star, moons orbiting rogue gas giants might harbor oceans of liquid water—and potentially complex life—for billions of years.
Liquid water is considered essential for life. Surprisingly, however, stable conditions that are conducive to life could exist far from any sun.
Look up on a clear night and you'll see the streaks of our modern satellite networks. What you don't see is the growing fallout for the atmosphere that keeps us alive.
A wave of satellite launches and reentries is changing the chemistry and physics of the middle and upper atmosphere. Studies warn of ozone depletion, stratospheric heating, and new metal aerosols from burning spacecraft.
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