Solar CNO neutrinos observed for the first time
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17:00 ‘Ghostly’ particles are proof of the secondary fusion process that powers our Sun Scientists who are members of the…
17:00 ‘Ghostly’ particles are proof of the secondary fusion process that powers our Sun Scientists who are members of the…
17:00 Der Borexino-Kollaboration, an der auch Wissenschaftler der TU Dresden beteiligt sind, ist es nach über 80 Jahren gelungen…
17:00 The Borexino collaboration, in which also scientists from TU Dresden are involved, has succeeded after more than 80 years…
The Borexino collaboration, in which also scientists from TU Dresden are involved, has succeeded after more than 80 years in…
‘Ghostly’ particles are proof of the secondary fusion process that powers our Sun Scientists who are members of the Borexino…
Stars are born in the collapse of massive clouds of gas and dust. Over their billions of years of existence, stars are fueled…
Die Sonne bezieht ihre Energie aus der Fusion von Wasserstoff zu Helium. Seit 1938 besagen Theorien jedoch, dass neben einer…
Neutrinos produced by the elusive carbon–nitrogen–oxygen (CNO) cycle in the Sun have been observed for the first time …
Embargoed until: Publicly released: 2020-11-26 03:00 Peer-reviewedWhat does this mean? Peer-reviewed: This work was reviewed…
In a landmark finding published Wednesday, scientists in Italy confirm the process that powers most stars.
AMHERST, Mass. - An international team of about 100 scientists of the Borexino Collaboration, including particle physicist…
Scientists who are members of the Borexino Collaboration have provided the first experimental proof of the occurrence of the so-c…
Stars produce their energy through nuclear fusion by converting hydrogen into helium - a process known to researchers as "hydroge…
An international team of about 100 scientists of the Borexino Collaboration, including particle physicist Andrea Pocar at the…
For the first time, scientists have detected neutrinos coming from the Sun’s core that got their start via the CNO process, an…
Deep within the Sun, high temperatures and pressures drive the fusion of hydrogen into helium.
Una grande avventura scientifica sta per concludersi. Dopo 13 anni intensi di operatività, in cui non sono mancate le sorprese, è…