Solar neutrinos trigger rare atomic reaction in underground detector

Researchers using the SNO+ detector in Canada have observed solar neutrinos converting carbon-13 into nitrogen-13, marking one of the lowest-energy neutrino interactions detected. This achievement relied on tracking paired light bursts separated by minutes. The finding builds on prior neutrino research that earned a Nobel Prize.

Neutrinos, elusive particles produced in the Sun's core, rarely interact with matter, earning them the nickname 'ghost particles.' In a breakthrough, scientists at the SNO+ experiment captured these particles inducing a transformation in carbon atoms deep underground.

The SNO+ detector, located two kilometers below ground at SNOLAB in Sudbury, Canada, shields sensitive measurements from cosmic rays. Operating in an active mine, it uses a liquid scintillator containing carbon-13 to detect interactions. The team employed a 'delayed coincidence' method, identifying events through an initial light flash from a neutrino striking a carbon-13 nucleus, followed by a second flash from the decay of the resulting radioactive nitrogen-13 after about ten minutes.

Data collection spanned 231 days, from May 4, 2022, to June 29, 2023, yielding 5.6 such events—aligning closely with the predicted 4.7 from solar neutrinos. This observation provides the first direct measurement of the cross-section for this reaction to nitrogen-13's ground state.

Lead author Gulliver Milton, a PhD student at the University of Oxford's Department of Physics, stated: "Capturing this interaction is an extraordinary achievement. Despite the rarity of the carbon isotope, we were able to observe its interaction with neutrinos, which were born in the Sun's core and traveled vast distances to reach our detector."

Co-author Professor Steven Biller added: "Solar neutrinos themselves have been an intriguing subject of study for many years, and the measurements of these by our predecessor experiment, SNO, led to the 2015 Nobel Prize in physics. It is remarkable that our understanding of neutrinos from the Sun has advanced so much that we can now use them for the first time as a 'test beam' to study other kinds of rare atomic reactions!"

SNO+ succeeds the SNO experiment, which resolved the solar neutrino problem and contributed to the 2015 Nobel Prize awarded to Arthur B. McDonald. SNOLAB staff scientist Dr. Christine Kraus noted: "This discovery uses the natural abundance of carbon-13 within the experiment's liquid scintillator to measure a specific, rare interaction... these results represent the lowest energy observation of neutrino interactions on carbon-13 nuclei to date."

These results, published in Physical Review Letters in 2025, open doors to studying other low-energy neutrino processes, enhancing insights into stellar nuclear fusion and cosmic evolution.

관련 기사

An international team of physicists, including Rutgers researchers, has concluded that a hypothesized fourth type of neutrino, known as the sterile neutrino, likely does not exist. Using the MicroBooNE experiment at Fermilab, they analyzed data from two neutrino beams over ten years and found no evidence for it with 95% certainty. The findings, published in Nature, challenge previous explanations for unusual neutrino behavior.

AI에 의해 보고됨

Physicists from the KATRIN collaboration have reported no evidence for a sterile neutrino in a precise analysis of tritium decay data. The findings, published in Nature, contradict earlier experimental claims and strengthen the case against a fourth neutrino type. The experiment, based in Germany, continues to gather more data for further tests.

중국 스폴레이션 중성자원(CSNS)은 2단계 건설에서 중요한 이정표를 달성했다. 첫 번째 빔라인인—중성자 기술 개발 스테이션—이 중성자 빔을 성공적으로 생산했다. 이는 빔라인의 장비 개발 및 설치 완료를 의미한다. 광동성 동관시에 위치한 이 시설은 슈퍼 현미경처럼 작동하며, 중성자를 이용해 재료를 조사하고 재생에너지, 항공우주, 생명과학 분야의 돌파구를 지원한다.

AI에 의해 보고됨

Astronomers have observed dramatic changes in the neutron star P13 over a decade, as it transitioned from a faint state to high luminosity. Located in the galaxy NGC 7793, about 10 million light-years away, P13's X-ray output and rotation rate shifted significantly. These observations provide new insights into supercritical accretion processes.

 

 

 

이 웹사이트는 쿠키를 사용합니다

사이트를 개선하기 위해 분석을 위한 쿠키를 사용합니다. 자세한 내용은 개인정보 보호 정책을 읽으세요.
거부