scholarly journals QED theory of the normal mass shift in few-electron atoms

2020 ◽  
Vol 101 (5) ◽  
Author(s):  
A. V. Malyshev ◽  
I. S. Anisimova ◽  
D. A. Glazov ◽  
M. Y. Kaygorodov ◽  
D. V. Mironova ◽  
...  
Keyword(s):  
Mass Shift ◽  
Normal Mass

scholarly journals Invisible neutrino decay: first vs second oscillation maximum

2021 ◽  
Vol 2021 (5) ◽  
Author(s):  
Kaustav Chakraborty ◽  
Debajyoti Dutta ◽  
Srubabati Goswami ◽  
Dipyaman Pramanik
Keyword(s):  
Decay Rate ◽  
Survival Probability ◽  
Mixing Angle ◽  
Decay Lifetime ◽  
Long Baseline ◽  
Physics Potential ◽  
Normal Mass ◽  
Compare And Contrast ◽  
Neutrino Decay ◽  
Oscillation Maximum

Abstract We study the physics potential of the long-baseline experiments T2HK, T2HKK and ESSνSB in the context of invisible neutrino decay. We consider normal mass ordering and assume the state ν3 as unstable, decaying into sterile states during the flight and obtain constraints on the neutrino decay lifetime (τ3). We find that T2HK, T2HKK and ESSνSB are sensitive to the decay-rate of ν3 for τ3/m3 ≤ 2.72 × 10−11s/eV, τ3/m3 ≤ 4.36 × 10−11s/eV and τ3/m3 ≤ 2.43 × 10−11s/eV respectively at 3σ C.L. We compare and contrast the sensitivities of the three experiments and specially investigate the role played by the mixing angle θ23. It is seen that for experiments with flux peak near the second oscillation maxima, the poorer sensitivity to θ23 results in weaker constraints on the decay lifetime. Although, T2HKK has one detector close to the second oscillation maxima, having another detector at the first oscillation maxima results in superior sensitivity to decay. In addition, we find a synergy between the two baselines of the T2HKK experiment which helps in giving a better sensitivity to decay for θ23 in the higher octant. We discuss the octant sensitivity in presence of decay and show that there is an enhancement in sensitivity which occurs due to the contribution from the survival probability Pμμ is more pronounced for the experiments at the second oscillation maxima. We also obtain the combined sensitivity of T2HK+ESSνSB and T2HKK+ESSνSB as τ3/m3 ≤ 4.36 × 10−11s/eV and τ3/m3 ≤ 5.53 × 10−11s/eV respectively at 3σ C.L.

scholarly journals Analysis of mass shift due to weak interactions

1974 ◽  
Vol 74 (3) ◽  
pp. 397-421 ◽  
Author(s):  
Fayyazuddin ◽  
Riazuddin
Keyword(s):  
Weak Interactions ◽  
Mass Shift

scholarly journals One-loop mass shift formula for kinks and self-dual vortices

2006 ◽  
Vol 39 (21) ◽  
pp. 6463-6471 ◽  
Author(s):  
A Alonso Izquierdo ◽  
W Garcia Fuertes ◽  
M de la Torre Mayado ◽  
J Mateos Guilarte
Keyword(s):  
Mass Shift

Trajectory and Mass Shift of a Classical Electron in a Radiation Pulse

1968 ◽  
Vol 176 (5) ◽  
pp. 1570-1573 ◽  
Author(s):  
Joseph H. Eberly ◽  
Arthur Sleeper
Keyword(s):  
Radiation Pulse ◽  
Mass Shift ◽  
Classical Electron

NEUTRINO OSCILLATION IN SUPERNOVA AND GRB NUCLEOSYNTHESIS

2008 ◽  
Vol 23 (17n20) ◽  
pp. 1409-1418 ◽  
Author(s):  
TOSHITAKA KAJINO ◽  
TAKAHIRO SASAQUI ◽  
TAKASHI YOSHIDA ◽  
WAKO AOKI
Keyword(s):  
Black Hole ◽  
Gamma Ray ◽  
Light Element ◽  
Core Collapse ◽  
Mass Hierarchy ◽  
Solar Abundance ◽  
Abundance Pattern ◽  
Mixing Angle ◽  
Normal Mass ◽  
Supernova Explosions

Neutrinos play the critical roles in nucleosyntheses of light-to-heavy mass elements in core-collapse supernovae (SNe). The light element synthesis is affected strongly by neutrino oscillations (MSW effect) through the ν-process in outer layers of supernova explosions. Specifically the 7 Li and 11 B yields increase by factors of 1.9 and 1.3 respectively in the case of large mixing angle solution, normal mass hierarchy, and sin 2 2θ13 = 2 × 10−3 compared to those without the oscillations. In the case of inverted mass hierarchy or nonadiabatic 13-mixing resonance, the increment of their yields is much smaller. We thus propose that precise constraint on mass hierarchy and sin 2 2θ13 is given by future observations of Li / B ratio or Li abundance in stars and presolar grains which are made from supernova ejecta. Gamma ray burst (GRB) nucleosynthesis in contrast is not affected strongly by thermal neutrinos from the central core which culminates in black hole (BH), although the effect of neutrinos from proto-neutron star prior to black hole formation is still unknown. We calculate GRB nucleosynthesis by turning off the thermal neutrinos and find that the abundance pattern is totally different from ordinary SN nucleosynthesis which satisfies the universality to the solar abundance pattern.

scholarly journals Hearts late after fontan operation have normal mass, normal volume, and reduced systolic function

2003 ◽  
Vol 42 (6) ◽  
pp. 1061-1065 ◽  
Author(s):  
Andreas Eicken ◽  
Sohrab Fratz ◽  
Christine Gutfried ◽  
Gunter Balling ◽  
Markus Schwaiger ◽  
...  
Keyword(s):  
Systolic Function ◽  
Fontan Operation ◽  
Normal Mass
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