1,690 research outputs found

    Three flavor neutrino oscillations in matter

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    We derive analytic expressions for three flavor neutrino oscillations in the presence of matter in the plane wave approximation using the Cayley-Hamilton formalism. Especially, we calculate the time evolution operator in both flavor and mass bases. Furthermore, we find the transition probabilities, matter mass squared differences, and matter mixing angles all expressed in terms of the vacuum mass squared differences, the vacuum mixing angles, and the matter density. The conditions for resonance in the presence of matter are also studied in some examples.Comment: 25 pages, 6 figures (PostScript), RevTe

    Dynamics of Natural Killer cell receptor revealed by quantitative analysis of photoswitchable protein

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    Natural Killer (NK) cell activation is dynamically regulated by numerous activating and inhibitory surface receptors that accumulate at the immune synapse. Quantitative analysis of receptor dynamics has been limited by methodologies which rely on indirect measurements such as fluorescence recovery after photobleaching. Here, we report a novel approach to study how proteins traffic to and from the immune synapse using NK cell receptors tagged with the photoswitchable fluorescent protein tdEosFP, which can be irreversibly photoswitched from a green to red fluorescent state by ultraviolet light. Thus, following a localized switching event, the movement of the photoswitched molecules can be temporally and spatially resolved by monitoring fluorescence in two regions of interest. By comparing images with mathematical models, we evaluated the diffusion coefficient of the receptor KIR2DL1 (0.23 +- 0.06 micron^2/s) and assessed how synapse formation affects receptor dynamics. Our data conclude that the inhibitory NK cell receptor KIR2DL1 is continually trafficked into the synapse and remains surprisingly stable there. Unexpectedly however, in NK cells forming synapses with multiple target cells simultaneously, KIR2DL1 at one synapse can relocate to another synapse. Thus, our results reveal a previously undetected inter-synaptic exchange of protein.Comment: 25 pages, 5 figure

    Effect of the 24 September 2011 solar radio burst on precise point positioning service

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    An intense solar radio burst occurred on 24 September 2011, which affected the tracking of Global Navigation Satellite Systems’ (GNSS) signals by receivers located in the sunlit hemisphere of the Earth. This manuscript presents for the first time the impacts of this radio burst on the availability of Fugro’s real-time precise point positioning service for GNSS receivers and on the quality of the L band data link used to broadcast this service. During the peak of the radio burst (12:50–13:20 UT), a reduction in the L band signal-to-noise ratio (SNR) is observed. For some receiver locations, a reset in the position filter is observed, which can be either due to the reduction in the L band SNR or the reduction in the number of tracked GNSS satellites. This reset in the position filter is accompanied by degradation in the positioning accuracy, which is also discussed herein

    A massa dos neutrinos. Teoria versus experimento.

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    Nas Ășltimas dĂ©cadas, soluçÔes ao problema do neutrino solar tĂȘm sido investigadas no contexto de teorias nas quais os neutrinos tĂȘm massa e podem oscilar entre os sabores eletrĂŽnico, muĂŽnico e tauĂŽnico. Os dados experimentais, hoje, parecem indicar que os neutrinos tĂȘm massa e que oscilaçÔes entre sabores realmente acontecem. No presente trabalho, efetuaremos uma revisĂŁo geral sobre a fĂ­sica de neutrinos desde a Ă©poca da proposta de sua existĂȘncia, apresentaremos suas propriedades e uma breve discussĂŁo das interaçÔes entre neutrinos e as outras partĂ­culas elementares no contexto do modelo padrĂŁo das interaçÔes fundamentais. Uma visĂŁo geral dos principais mecanismos de produção de neutrinos no interior solar, o espectro de energia destes neutrinos, os mĂ©todos de detecção de neutrinos e as caracterĂ­sticas dos principais detectores existentes serĂŁo apresentados. No contexto de teorias envolvendo neutrinos massivos, mostraremos como o fluxo de neutrinos solares pode ser afetado devido a oscilaçÔes entre sabores de neutrinos. Alguns dados experimentais e as conclusĂ”es que podemos tirar do confronto entre estes dados e a hipĂłtese de oscilaçÔes entre sabores serĂŁo tambĂ©m apresentados

    The Heat Distribution of the Underdamped Langevin Equation

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    In the Stochastic Thermodynamics theory, heat is a random variable with a probability distribution associated. Studies in the distribution of heat are mostly in the overdamped regime. Here we solve the heat distribution in the underdamped regime for three different cases: the free particle, the linear potential, and the harmonic potential. The results are exact and generalize known results in the literature.Comment: 19 pages, 9 subfigure
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