Neutrino/Bibliography: Difference between revisions
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*[http://nobelprize.org/nobel_prizes/physics/laureates/1945/pauli-bio.html Biography of Wolfgang Pauli on the Nobel Prize website]. | |||
*[http://nobelprize.org/nobel_prizes/physics/laureates/1938/fermi.html Biography of Enrico Fermi on the Nobel Prize website]. | |||
*[http://www-numi.fnal.gov/public/story.html The Story of the Neutrino]. NuMI-MINOS Homepage. Fermi National Accelerator Laboratory. | |||
*Graciela B. Gelmini, Alexander Kusenko, Thomas J. Weiler. (2010) [http://bit.ly/bN41ra Through Neutrino Eyes]. ''Scientific American''. May 2010. Pp. 38-45. [http://www.scientificamerican.com/article.cfm?id=through-neutrino-eyes Preview of Article]. | *Graciela B. Gelmini, Alexander Kusenko, Thomas J. Weiler. (2010) [http://bit.ly/bN41ra Through Neutrino Eyes]. ''Scientific American''. May 2010. Pp. 38-45. [http://www.scientificamerican.com/article.cfm?id=through-neutrino-eyes Preview of Article]. | ||
**"Neutrinos are no longer just a curiosity of physics but a practical tool for astronomy...Neutrinos will give astronomers a type of x-ray vision far better than actual x-rays. Being the most unreactive type of subatomic particle, they pass through intervening matter as though it were hardly there—revealing the cores of stars and other dramatic but otherwise hidden places in the cosmos." | **"Neutrinos are no longer just a curiosity of physics but a practical tool for astronomy...Neutrinos will give astronomers a type of x-ray vision far better than actual x-rays. Being the most unreactive type of subatomic particle, they pass through intervening matter as though it were hardly there—revealing the cores of stars and other dramatic but otherwise hidden places in the cosmos." | ||
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*Faye Flam (2010) [http://www.physorg.com/news199380378.html Physicists hunt for a trace of the elusive, invisible geoneutrino]. PhysOrg.com. | *Faye Flam (2010) [http://www.physorg.com/news199380378.html Physicists hunt for a trace of the elusive, invisible geoneutrino]. PhysOrg.com. | ||
*Allen SW, Schmidtn RW, Bridle SL. (2008) [http://arxiv.org/abs/astro-ph/0306386 A preference for a non-zero neutrino mass from cosmological data]. | |||
**"We present results from the analysis of cosmic microwave background (CMB), large scale structure (galaxy redshift survey) and X-ray galaxy cluster (baryon fraction and X-ray luminosity function) data, assuming a geometrically flat cosmological model and allowing for tensor components and a non-negligible neutrino mass. From a combined analysis of all data, assuming three degenerate neutrinos species, we measure a contribution of neutrinos to the energy density of the universe, Ω<sub>ν</sub>h<sup>2</sup> = 0.0059(+0.0033;−0.0027)(68 per cent confidence limits), with zero falling on the 99 per cent confidence limit. This corresponds to ~4 per cent of the total mass density of the Universe and implies a species-summed neutrino mass Σ<sub><i>i</i></sub><i>m</i><sub><i>i</i></sub> = 0.56(+0.30;−0.26)eV, or <i>m</i><sub><i>i</i></sub> = 0.2eV per neutrino." | |||
*Lopes I, Silk J. (2010) [http://www.sciencemag.org/cgi/content/abstract/330/6003/462 Neutrino Spectroscopy Can Probe the Dark Matter Content in the Sun]. ''Science'' 330:462. | Neutrino flux variations in the sun as a measure of the sun's content of dark matter. | |||
*Halzen F. (2007) [http://dx.doi.org/10.1126/science.1136504 Neutrino Astrophysics Experiments Beneath the Sea and Ice]. ''Science'' 315:66-68. | Describes the basic requirements for construction of a neutrino telescope. | |||
*Fiorentini G, Lissia M, Mantovani F, Vannucci R. 2005) [http://dx.doi.org/10.1016/j.nuclphysbps.2005.03.019 A brief review on geo-neutrinos]. ''Nuclear Physics B - Proceedings Supplements'' 145:170–173. | |||
**<font face=”Gill Sans MT”><u>Abstract</u>:The detection of neutrinos from U, Th, and K decay in the Earth (geo-neutrinos) will help to fix the total amount of long-lived radioactive elements and thus the radiogenic contribution to the terrestrial heat. Moreover, it will provide a direct test of a fundamental paradigm about the origin, formation and structure of the Earth, i.e., the Bulk Silicate Earth model. Alternative or variant models of Earth (including the presence of potassium or the possibility of a giant reactor in the core) can also be checked. This short review presents the status and prospects in this exciting field of research.</font> | |||
Latest revision as of 16:55, 14 January 2013
- Please sort and annotate in a user-friendly manner. For formatting, consider using automated reference wikification.
- The Story of the Neutrino. NuMI-MINOS Homepage. Fermi National Accelerator Laboratory.
- Graciela B. Gelmini, Alexander Kusenko, Thomas J. Weiler. (2010) Through Neutrino Eyes. Scientific American. May 2010. Pp. 38-45. Preview of Article.
- "Neutrinos are no longer just a curiosity of physics but a practical tool for astronomy...Neutrinos will give astronomers a type of x-ray vision far better than actual x-rays. Being the most unreactive type of subatomic particle, they pass through intervening matter as though it were hardly there—revealing the cores of stars and other dramatic but otherwise hidden places in the cosmos."
- Radioactivity. (2010). In Encyclopædia Britannica. Retrieved July 12, 2010, from Encyclopædia Britannica Online.
- Faye Flam (2010) Physicists hunt for a trace of the elusive, invisible geoneutrino. PhysOrg.com.
- Allen SW, Schmidtn RW, Bridle SL. (2008) A preference for a non-zero neutrino mass from cosmological data.
- "We present results from the analysis of cosmic microwave background (CMB), large scale structure (galaxy redshift survey) and X-ray galaxy cluster (baryon fraction and X-ray luminosity function) data, assuming a geometrically flat cosmological model and allowing for tensor components and a non-negligible neutrino mass. From a combined analysis of all data, assuming three degenerate neutrinos species, we measure a contribution of neutrinos to the energy density of the universe, Ωνh2 = 0.0059(+0.0033;−0.0027)(68 per cent confidence limits), with zero falling on the 99 per cent confidence limit. This corresponds to ~4 per cent of the total mass density of the Universe and implies a species-summed neutrino mass Σimi = 0.56(+0.30;−0.26)eV, or mi = 0.2eV per neutrino."
- Lopes I, Silk J. (2010) Neutrino Spectroscopy Can Probe the Dark Matter Content in the Sun. Science 330:462. | Neutrino flux variations in the sun as a measure of the sun's content of dark matter.
- Halzen F. (2007) Neutrino Astrophysics Experiments Beneath the Sea and Ice. Science 315:66-68. | Describes the basic requirements for construction of a neutrino telescope.
- Fiorentini G, Lissia M, Mantovani F, Vannucci R. 2005) A brief review on geo-neutrinos. Nuclear Physics B - Proceedings Supplements 145:170–173.
- Abstract:The detection of neutrinos from U, Th, and K decay in the Earth (geo-neutrinos) will help to fix the total amount of long-lived radioactive elements and thus the radiogenic contribution to the terrestrial heat. Moreover, it will provide a direct test of a fundamental paradigm about the origin, formation and structure of the Earth, i.e., the Bulk Silicate Earth model. Alternative or variant models of Earth (including the presence of potassium or the possibility of a giant reactor in the core) can also be checked. This short review presents the status and prospects in this exciting field of research.