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Mass-radius Relations for Helium White Dwarfs
Mass-radius Relations for Helium White Dwarfs

Weak interactions and nonconservation of parity
Weak interactions and nonconservation of parity

The top quark
The top quark

Elemental Synthesis in the Universe
Elemental Synthesis in the Universe

PANDA - Particles And Non-Destructive Analysis
PANDA - Particles And Non-Destructive Analysis

Impact of Large-Mixing-Angle Neutrino Oscillations
Impact of Large-Mixing-Angle Neutrino Oscillations

... Figure 4-2. In (i), only the quarks directly involved in the neutron decay reaction shown in Figure 4-1 are focused. In nature, it is known that not only the reaction (i), but also reactions (ii) and (iii) occur. All the reactions proceed from left to right. In (ii), a reaction is shown in which an ...
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334 kb

The current status of ”Troitsk nu-mass”
The current status of ”Troitsk nu-mass”

Fundamental interactions
Fundamental interactions

... However, information on the g-factor of the bound electron in hydrogen-like ions was until recently available only for the hydrogen atom and the 4He+-ion. For the determination of the g-factor of the bound electron in highly charged ions as a test of bound-state QED a precision Penning trap has been ...
ICHEP_2010_Electroweak_Stars
ICHEP_2010_Electroweak_Stars

ppt
ppt

6 Weak Interactions
6 Weak Interactions

pbarp - CERN Indico
pbarp - CERN Indico

enlargement
enlargement

All three experiments have identified specific B meson decays and
All three experiments have identified specific B meson decays and

Fluorine nucleosynthesis
Fluorine nucleosynthesis

The NEXT experiment
The NEXT experiment

Document
Document

Aran Sivaguru Dissertation
Aran Sivaguru Dissertation

Report - Nevis Laboratories
Report - Nevis Laboratories

... There are three main sources of neutrinos. High energy neutrinos (10 MeV - 100 GeV) can be made in particle accelerators by aiming a proton beam onto a target. Lower energy (≈ 4 MeV) anti-neutrinos are produced from the decay of neutron rich fission fragments in nuclear reactors. The main source of ...
first determination of the proton`s weak charge
first determination of the proton`s weak charge

Tasevsky_RECFA_270315
Tasevsky_RECFA_270315

Plasma_02 - StealthSkater
Plasma_02 - StealthSkater

... [Jonas Schultz] (University of California, Irvine): They concluded that it was a practical impossibility - that no one would ever see these neutrinos. And I think that's what put people off for many years from even trying. [Narrator]: But according to Pauli, neutrinos were produced when atomic nucle ...
arXiv:1606.09570v1 [physics.gen-ph] 29 Jun 2016
arXiv:1606.09570v1 [physics.gen-ph] 29 Jun 2016

Colloquium Slides
Colloquium Slides

< 1 2 3 4 5 6 7 8 9 10 12 >

Faster-than-light neutrino anomaly



In 2011, the OPERA experiment mistakenly observed neutrinos appearing to travel faster than light. Even before the mistake was discovered, the result was considered anomalous because speeds higher than that of light in a vacuum are generally thought to violate special relativity, a cornerstone of the modern understanding of physics for over a century.OPERA scientists announced the results of the experiment in September 2011 with the stated intent of promoting further inquiry and debate. Later the team reported two flaws in their equipment set-up that had caused errors far outside their original confidence interval: a fiber optic cable attached improperly, which caused the apparently faster-than-light measurements, and a clock oscillator ticking too fast. The errors were first confirmed by OPERA after a ScienceInsider report; accounting for these two sources of error eliminated the faster-than-light results.In March 2012, the collocated ICARUS experiment reported neutrino velocities consistent with the speed of light in the same short-pulse beam OPERA had measured in November 2011. ICARUS used a partly different timing system from OPERA and measured seven different neutrinos. In addition, the Gran Sasso experiments BOREXINO, ICARUS, LVD and OPERA all measured neutrino velocity with a short-pulsed beam in May, and obtained agreement with the speed of light.On June 8, 2012 CERN research director Sergio Bertolucci declared on behalf of the four Gran Sasso teams, including OPERA, that the speed of neutrinos is consistent with that of light. The press release, made from the 25th International Conference on Neutrino Physics and Astrophysics in Kyoto, states that the original OPERA results were wrong, due to equipment failures.On July 12, 2012 OPERA updated their paper by including the new sources of errors in their calculations. They found agreement of neutrino speed with the speed of light.
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