Question
One type of these bodies ceases to emit radiation at the so-called “death line.” A 2017 multi-messenger astronomy breakthrough involved measuring both gravitational waves and a gamma-ray burst from the merger of two of these bodies, known as a kilonova. An upper limit on these bodies’ mass is named for Tolman, Oppenheimer, and Volkov. A “glitch” is a small increase in the frequency emitted by rapidly rotating examples of these bodies called pulsars. Stars whose mass is just above the Chandrasekar limit form one of these bodies after a supernova instead of a white dwarf. For 10 points, what extremely dense celestial bodies are named for a subatomic particle? ■END■
ANSWER: neutron stars [accept pulsars until read; reject “stars”]
<Other Science>
= Average correct buzz position
Summary
2024 ACF Fall at Cornell | fall | Y | 8 | 75% | 0% | 88% | 93.83 |
2024 ACF Fall at Ohio State | fall | Y | 8 | 100% | 0% | 63% | 84.88 |
2024 ACF Fall at Washington | fall | Y | 6 | 83% | 0% | 83% | 88.40 |
2024 ACF Fall at Georgia | fall | Y | 10 | 90% | 0% | 70% | 95.89 |
2024 ACF Fall at North Carolina | fall | Y | 9 | 56% | 0% | 89% | 97.40 |
2024 ACF Fall at Claremont Colleges | fall | Y | 5 | 100% | 0% | 60% | 89.40 |
2024 ACF Fall at Rutgers | fall | Y | 8 | 75% | 0% | 75% | 76.17 |
2024 ACF Fall at Illinois | fall | Y | 9 | 100% | 0% | 33% | 58.67 |
Buzzes
Player | Team | Opponent | Buzz Position | Value |
---|---|---|---|---|
Andrew Leffingwell | UW Sloth | UW Pride | 15 | -5 |
Carson Kessler | UW Lust | UBC B | 18 | -5 |
Alan Fan | UW Envy | Boise State | 32 | -5 |
Joyann Hua | UBC A | Alberta | 35 | -5 |
Andrea Yu | UW Chastity | UW Greed | 39 | -5 |
Dylan Bianchi | UW Greed | UW Chastity | 40 | 0 |
Matthew Wang | UBC B | UW Lust | 46 | 10 |
Darrien Liang | UW Wrath | UW Gluttony | 70 | 10 |
Kamil Swiatek | Alberta | UBC A | 108 | 10 |
Jacob Bieri | Boise State | UW Envy | 109 | 10 |
Luke Strole | UW Pride | UW Sloth | 109 | 10 |