Amanote Research

Amanote Research

    RegisterSign In

Why Is the Neutrino Oscillation Formula Expanded in Δm 21 2 /Δm 31 2 Still Accurate Near the Solar Resonance in Matter?

Journal of High Energy Physics - Germany
doi 10.1007/jhep10(2015)090
Full Text
Open PDF
Abstract

Available in full text

Categories
High Energy PhysicsNuclear
Date

October 1, 2015

Authors
Xun-Jie Xu
Publisher

Springer Science and Business Media LLC


Related search

Δm-Deferred Statistical Convergence of Order Α

Filomat
Mathematics
2016English

Soudan 2 Atmospheric Neutrino Oscillation Studies

2001English

Uncovering the Matter-Neutrino Resonance

Physical Review D
AstronomyPhysics
2016English

VEP Oscillation Solutions to the Solar Neutrino Problem

2000English

Pinning Down Neutrino Oscillation Parameters in the 2–3 Sector With a Magnetised Atmospheric Neutrino Detector: A New Study

European Physical Journal C
EngineeringAstronomyPhysics
2017English

The Atmospheric Neutrino Anomaly in Soudan 2

Nuclear Physics B - Proceedings Supplements
1995English

Front Matter, Vol. 21, Issue 2

Studies in 20th & 21st Century Literature
1997English

SN 1987A and the Status of Oscillation Solutions to the Solar Neutrino Problem

Physical Review D
2002English

PAS Volume 21 Issue 2 Front Matter

Publications of the Astronomical Society of Australia
AstrophysicsAstronomyPlanetary ScienceSpace
2004English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2025 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy