A Texas A&M University-led collaboration has yielded new insight into one of the universe’s most important primordial reactions that made all life on Earth possible.
The multi-institution team of nuclear scientists that also includes researchers from Washington University in St. Louis and Ohio University concluded in a recent study that the role neutrons play in the creation of carbon, considered the definitive building block of life, actually is much smaller than previously thought.
Their data, acquired during 2020 and analyzed within the past year, is detailed in a paper published in Nature Communications.
“These findings are extremely significant because it demonstrates that the rate at which stars burn helium together to form carbon is less sensitive to any neutrons in the stars, which were previously thought to speed up this process,” said Dr. Jack Bishop, an assistant research scientist at the Texas A&M Cyclotron Institute and a lead author of the paper. “Understanding the way that stars burn is extremely important in understanding the life and death of stars, as well as where the elements that make up our universe originate from and in what quantity.”









