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Neutrino Neutrino Neutrino

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Neutrinos are elusive, almost massless sub-atomic particles that travel just below light-speed, to which normal matter is transparent. A neutrino is probably a sub-atomic particle. According to the String Theory, neutrinos are composed mainly of porn. Recent updates suggest that there may be subatomic teenagers providing a sticky substance which holds the neutrinos together in an anti stable paradox. The controversy around this particle stems from the fact according to the String Theory, all sub-atomic particles are made of cheese. Proof of a non-cheese based variety would prove the String Theory wrong, thereby proving that the universe doesn't exist and also bringing the sexual orientation of your mom into question. It is first used in Golden Age 205. Neutrinos are particles that pass through any matter easily, no matter how dense. The Omeyocans were able to create an environment where neutrinos were slowed down. (SG1: "Crystal Skull") The Asgard utilized neutrino-ion generators, which put out 1 billion kilojoules of energy per second - one terawatt (for comparison, the total power usage of humans worldwide was 16 TW in 2006, and the average lightning strike peaks at 1 TW). (SG1: "Nemesis") Neutrinos are subatomic particles which can be used for a variety of purposes. Federation starships have neutrino detectors included in there sensor arrays, and the presence of elevated neutrino levels could indicate the presence of a ship, possibly cloaked. The antiparticle of the neutrino is the antineutrino. A phenomenon of neutrinos forming a spherical shape is a neutrino bubble. (VOY episode: "Prime Factors") Neutrino (1): Bob Wiltfong, Steve Buck, Chris DeLuca, Dyna Moe, Kurt Braunholer, Sean Cordobes, Marc Campbell, Carl Hagen, Patrick Birch Neutrino (2): Bob Wiltfong, Steve Buck, Chris DeLuca, Kurt Braunholer, Sean Cordobes, Marc Campbell, Carl Hagen, Patrick Birch Neutrino (3): Bob Wiltfong, Steve Buck, Chris DeLuca, Jessica Allen, Kurt Braunholer, Ptolemy Slocum, Marc Campbell, Patrick Birch Neutrino (4): Bob Wiltfong, Steve Buck, Chris DeLuca, Jessica Allen, Kurt Braunholer, Ptolemy Slocum, Patrick Birch, Suzanne Shepard Neutrino (5): Bob Wiltfong, Steve Buck, Jessica Allen, Kurt Braunholer, Ptolemy Slocum, Suzanne Shepard, Jayne Napier, Jen Nails Neutrino (6): Bob Wiltfong, Steve Buck, Jessica Allen, Kurt Braunholer, Ptolemy Slocum, Jen Nails, Rebekka Johnson, Matt Donnelly Neutrin Neutrino sind subatomare Elementarteilchen, welche die Sternenflotte in verschiedenen Anwendungsgebieten nutzt. In der realen Wissenschaft zählen Neutrinos zur Teilchenfamilie der Leptonen. Es gibt insgesamt 3 verschiedene Generationen von Neutrinos, das Elektron-Neutrino, das Myon-Neutrino und das Tau-Neutrino. Neutrinos haben praktisch keine nennenswerte Masse und interagieren sogut wie garnicht mit Materie. Sie entstehen als Nebenprodukt bei Kernumwandlungsprozessen wie z.B. Kernfusion. Auch Raumschiffe hinterlassen Neutrinoemissionen: The presence of elevated neutrinos may indicate the presence of a ship – possibly cloaked. The Bajoran wormhole also emitted neutrinos before opening, giving Deep Space 9 a moment to prepare before any ship came through. Neutrino is a planet appearing in the IDW comics. It's the home of the Neutrinos. In the 1987 TMNT cartoon, the Neutrinos' home planet was shown, but it's name was never mentioned. In 1931, Nuclear Theorist Wolfgang Pauli, basing his prediction on the fact that energy and momentum did not appear to be conserved in certain radioactive decays, hypothsizes the idea of a new sub-atomic particle.This new particle carries off energy lost in the decay of certain atoms. Three years later in 1934, on of the future Manhattan Project members, Enrico Fermi, further investigates, and subsequently strengthens the possibility of the hypothesized particle. Fermi in fact invents the term Neutrino, which in Italian means little neutral one. Fermi is the first in a list of many physicists to ad to the theory of the Neutrino. Neutrino is the name for the QNX microkernel operating system. The Neutrino name is used for all 6.x versions of QNX. Neutrino includes: * A Realtime microkernel * Resource manager architecture * Standard device drivers * Standard POSIX libraries and utilities * Standard file systems * Package management file system Neutrino är partiklar som passerar genom alla ärenden enkelt, oavsett hur tät. Omeyocaner kunde skapa en miljö där neutrino har mattats av. (SG1: "Crystal Skull") Asgard utnyttjar neutrino-jon-generatorer, som lagt ut en miljard kilojoule energi per sekund. (SG1: "Nemesis") kategori:Partiklar Neutrinos were near massless particles emitted by stars. They were utilized with neutrino radiators. Gotals had the ability to sense them, whereas most other beings could not.

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It is first used in Golden Age 205. Neutrinos are particles that pass through any matter easily, no matter how dense. The Omeyocans were able to create an environment where neutrinos were slowed down. (SG1: "Crystal Skull") The Asgard utilized neutrino-ion generators, which put out 1 billion kilojoules of energy per second - one terawatt (for comparison, the total power usage of humans worldwide was 16 TW in 2006, and the average lightning strike peaks at 1 TW). (SG1: "Nemesis") Neutrino sind subatomare Elementarteilchen, welche die Sternenflotte in verschiedenen Anwendungsgebieten nutzt. In der realen Wissenschaft zählen Neutrinos zur Teilchenfamilie der Leptonen. Es gibt insgesamt 3 verschiedene Generationen von Neutrinos, das Elektron-Neutrino, das Myon-Neutrino und das Tau-Neutrino. Neutrinos haben praktisch keine nennenswerte Masse und interagieren sogut wie garnicht mit Materie. Sie entstehen als Nebenprodukt bei Kernumwandlungsprozessen wie z.B. Kernfusion. Sterne erzeugen sogenannte solare Neutrinos. Normalerweise sind sie so verteilt, dass die Hälfte von ihnen in eine Richtung und die andere Hälfte in die Gegenrichtung rotiert (Stichwort: Spin). Durch Beeinflussung von einem fremden Spielgerät, welches die Gesetze der Wahrscheinlichkeit manipuliert, rotieren 2370 jedoch 90% der solaren Neutrinos auf Deep Space 9 nur in eine Richtung. Auf diese Art und Weise kann Jadzia Dax diese Manipulation aufdecken und viele seltsame Vorkommnisse auf der Raumstation erklären. (DS9: ) Neutrinos sind in Wirklichkeit alle linksdrehend. Im Star Trek Science Logs nimmt der Autor und theoretische Physiker Lawrence Krauss die Schuld für diesen Fehler auf sich, da er davon ausging, dass Neutrinos wie andere subatomare Partikel in beide Richtungen rotieren würden, ohne dies zu überprüfen. Der metaphasische Schutzschild benutzt ein Subraumfeld. Gerät dieses Feld in Kontakt mit dem Plasma einer Korona, erzeugt es einen erhöhten Neutrinowert. (TNG: ) Das Dal'Rok, das jedes Jahr zum Ende der Erntezeit über ein bajoranisches Dorf hereinfällt und dass vom Sirah mit Hilfe eines Drehkörperfragments geschaffen worden ist, hinterlässt Neutrinospuren, wenn es im Dorf wütet. (DS9: ) Auch Raumschiffe hinterlassen Neutrinoemissionen: * 2371 kann die durch Thomas Riker entführte USS Defiant trotz aktivierter Tarnvorrichtung geortet werden, weil eine Warpgondel ein Neutrinoleck aufweist. (DS9: ) * 2373 nutzt Michael Eddington eine Sonde mit falschen Neutrinowerten, um ein Raumschiff vorzutäuschen. (DS9: ) * Als 2374 die Flotte des Dominions innerhalb des bajoranischen Wurmloches verschwindet, registriert Jadzia Dax anschließend keine Neutrinowerte mehr auf den Sensoren. (DS9: ) A neutrino is probably a sub-atomic particle. According to the String Theory, neutrinos are composed mainly of porn. Recent updates suggest that there may be subatomic teenagers providing a sticky substance which holds the neutrinos together in an anti stable paradox. The controversy around this particle stems from the fact according to the String Theory, all sub-atomic particles are made of cheese. Proof of a non-cheese based variety would prove the String Theory wrong, thereby proving that the universe doesn't exist and also bringing the sexual orientation of your mom into question. Neutrino is the name for the QNX microkernel operating system. The Neutrino name is used for all 6.x versions of QNX. Neutrino includes: * A Realtime microkernel * Resource manager architecture * Standard device drivers * Standard POSIX libraries and utilities * Standard file systems * Package management file system Neutrino är partiklar som passerar genom alla ärenden enkelt, oavsett hur tät. Omeyocaner kunde skapa en miljö där neutrino har mattats av. (SG1: "Crystal Skull") Asgard utnyttjar neutrino-jon-generatorer, som lagt ut en miljard kilojoule energi per sekund. (SG1: "Nemesis") kategori:Partiklar Neutrinos are elusive, almost massless sub-atomic particles that travel just below light-speed, to which normal matter is transparent. Neutrino is a planet appearing in the IDW comics. It's the home of the Neutrinos. In the 1987 TMNT cartoon, the Neutrinos' home planet was shown, but it's name was never mentioned. Neutrinos are subatomic particles which can be used for a variety of purposes. Federation starships have neutrino detectors included in there sensor arrays, and the presence of elevated neutrino levels could indicate the presence of a ship, possibly cloaked. The antiparticle of the neutrino is the antineutrino. A phenomenon of neutrinos forming a spherical shape is a neutrino bubble. (VOY episode: "Prime Factors") Natural phenomena have also been known to produce neutrinos, such as the Bajoran wormhole. It was the detection of elevated neutrino levels that allowed a team from Deep Space 9 to discover the wormhole in the year 2369. (DS9 episode & novelization: Emissary) Following the disappearance of a Danube-class runabout carrying several Starfleet admirals near the Bajoran wormhole in 2370, Lieutenant Jadzia Dax noted that the neutrino output of the wormhole had become erratic. It was later discovered that it was due to interference by the Cardassians and the "Othersiders". (TNG - DS9: The Landmark Crossover comic: "Prophets and Losses") Neutrino (1): Bob Wiltfong, Steve Buck, Chris DeLuca, Dyna Moe, Kurt Braunholer, Sean Cordobes, Marc Campbell, Carl Hagen, Patrick Birch Neutrino (2): Bob Wiltfong, Steve Buck, Chris DeLuca, Kurt Braunholer, Sean Cordobes, Marc Campbell, Carl Hagen, Patrick Birch Neutrino (3): Bob Wiltfong, Steve Buck, Chris DeLuca, Jessica Allen, Kurt Braunholer, Ptolemy Slocum, Marc Campbell, Patrick Birch Neutrino (4): Bob Wiltfong, Steve Buck, Chris DeLuca, Jessica Allen, Kurt Braunholer, Ptolemy Slocum, Patrick Birch, Suzanne Shepard Neutrino (5): Bob Wiltfong, Steve Buck, Jessica Allen, Kurt Braunholer, Ptolemy Slocum, Suzanne Shepard, Jayne Napier, Jen Nails Neutrino (6): Bob Wiltfong, Steve Buck, Jessica Allen, Kurt Braunholer, Ptolemy Slocum, Jen Nails, Rebekka Johnson, Matt Donnelly Neutrino (7): Bob Wiltfong, Steve Buck, Jessica Allen, Kurt Braunholer, Ptolemy Slocum, Rebekka Johnson, Matt Donnelly, Rachel Biello CURRENT The presence of elevated neutrinos may indicate the presence of a ship – possibly cloaked. The Bajoran wormhole also emitted neutrinos before opening, giving Deep Space 9 a moment to prepare before any ship came through. In September 2011, the OPERA collaboration released calculations showing velocities of 17 GeV and 28 GeV neutrinos exceeding the speed of light in their experiments. On July 12, 2012 OPERA updated their paper by including the new sources of errors in their calculations. The literal meaning of neutrino is "the little neutral one". This particle was discovered by Earth scientists in 1956. The nuclear reactions of stars are a major source of neutrinos.(Star Trek Encyclopedia (4th ed., vol. 2, p. 77) ) Neutrinos were near massless particles emitted by stars. They were utilized with neutrino radiators. Gotals had the ability to sense them, whereas most other beings could not. In 1931, Nuclear Theorist Wolfgang Pauli, basing his prediction on the fact that energy and momentum did not appear to be conserved in certain radioactive decays, hypothsizes the idea of a new sub-atomic particle.This new particle carries off energy lost in the decay of certain atoms. Three years later in 1934, on of the future Manhattan Project members, Enrico Fermi, further investigates, and subsequently strengthens the possibility of the hypothesized particle. Fermi in fact invents the term Neutrino, which in Italian means little neutral one. Fermi is the first in a list of many physicists to ad to the theory of the Neutrino. In 1959, Discovery of a particle fitting the expected characteristics of the neutrino is announced by Clyde Cowan and Fred Reines (a founding member of Super-Kamiokande; UCI professor emeritus and recipient of the 1995 Nobel Prize in physics for his contribution to the discovery). This neutrino is later determined to be the partner of the electron. Kamionade is the spearhead tool of the research following the Neutrino. Three years later, Experiments at Brookhaven National Laboratory and CERN, the European Laboratory for Nuclear Physics make a surprising discovery: neutrinos produced in association with muons do not behave the same as those produced in association with electrons. They have, in fact, discovered a second type of neutrino (the muon neutrino). The first experiment to detect neutrinos occurs in 1959, was produced by the Sun's burning, using a liquid Chlorine target deep underground, reports that less than half the expected neutrinos are observed. This is the origin of the long-standing "solar neutrino problem." The possibility that the missing electron neutrinos may have transformed into another type (undetectable to this experiment) is soon suggested, but unreliability of the solar model on which the expected neutrino rates are based is initially considered a more likely explanation. In 1978 The tau particle is discovered at SLAC, the Stanford Linear Accelerator Center. It is soon recognized to be a heavier version of the electron and muon, and its decay exhibits the same apparent imbalance of energy and momentum that led Pauli to predict the existence of the neutrino in 1931. The existence of a third neutrino associated with the tau is hence inferred, although this neutrino has yet to be directly observed. In 1985 The IMB experiment, a large water detector searching for proton decay but which also detects neutrinos, notices that fewer muon-neutrino interactions than expected are observed. The anomaly is at first believed to be an artifact of detector inefficiencies. That same yearA Russian team reports measurement, for the first time, of a non-zero neutrino mass. The mass is extremely small (10,000 times less than the mass of the electron), but subsequent attempts to independently reproduce the measurement do not succeed. Kamiokande, in 1987, another large water detector looking for proton decay, and IMB detect a simultaneous burst of neutrinos from Supernova 1987A. The next yearKamiokande, another water detector looking for proton decay but better able to distinguish muon neutrino interactions from those of electron neutrino, reports that they observe only about 60% of the expected number of muon-neutrino interactions. Three events followed in the year 1989, The Frejus and NUSEX experiments, much smaller than either Kamiokande or IMB, and using iron rather than water as the neutrino target, report no deficit of muon-neutrino interactions. Following this, Experiments at CERN's Large Electron-Positron (LEP) accelerator determine that no additional neutrinos beyond the three already known can exist. Later that year, Kamiokande becomes the second experiment to detect neutrinos from the Sun, and confirms the long-standing anomaly by finding only about 1/3 the expected rate. In 1990After an upgrade which improves the ability to identify muon-neutrino interactions, IMB confirms the deficit of muon neutrino interactions reported by Kamiokande. In 1994 Kamiokande finds a deficit of high-energy muon-neutrino interactions. Muon-neutrinos travelling the greatest distances from the point of production to the detector exhibit the greatest depletion. Later that year the Kamiokande and IMB groups collaborate to test the ability of water detectors to distinguish muon- and electron-neutrino interactions, using a test beam at the KEK accelerator laboratory. The results confirm the validity of earlier measurements. The two groups will go on to form the nucleus of the Super-Kamiokande project. In 1996, The Super-Kamiokande detector begins operation, leading the find in 1998, which announces evidence of non-zero neutrino mass at the Neutrino '98 conference.

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