SNOlab On October 27, 2008, Kevin Graham gave a seminar about an experiment called SNO Lab. When I first h atrial auricled about the seminar’s name, I conception the seminar was going to talk about “snow”, since I make out snow, I was excited. However when I arrived to the lecture, I was disappointed. As Mr. Graham, introduced himself and began to talk, my ear was attracted to what he was saying, neutrinos. Although I am non big strike out of neutrinos, it was very fascinating. Overall he was very good speaker with a broad knowledge. He began the lecture describing the function of neutrinos and it is situation in universe. After, he draw the temperateness, talked about the matter, and the description of SNO Lab. e + P+ = N (neutral) + e+ P+ + P+ = 2H + e- + e. When the sun is burning it forms nuclear coalition because it is using a dim nuclear force, so it has a weak interaction. When this process is proceeding, it produces life-t hreatening elements such as deuteron (2H), photons, and negatron neutrinos only. However, eventually photons and neutrinos leave the sun. So the experimentalist calamus Davis Jr and theorist tooshie Bahcall decided to work it out. Ray decided to do nigh underground Chloride experiment, which had a scurvy signal rate. Ve + d (proton neutron) = P + p + e- which only detects Ve.

However, when it is in neural current, {draw: shut in} Reference Giambattista A, B.M. Richardson, R.C. Richardson 2008. Physics, Mc Graw pile Higher Education. R1058-R1092 McMurray. J.E., R.C. Fay. 2008 Chemistry fifth part Edition, Pearson-! Prentice Hall. 930-932 Luis M. Luis. 2000. Four Fundamental Forces of Nature, astronomy Now Neutrino mass discovered, IOP make McKay. S. 2003. The Trouble with Oscillation, Neutrinos They Are very(prenominal) Small http://www.sallymckay.ca/oscillation/neutrinos.html Noble. T. 2005 SNO Lab, SNO LabIf you want to put a full essay, order it on our website:
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