Amanote Research

Amanote Research

    RegisterSign In

Do Solar Models With Weakly Interacting Massive Particles Reproduce the Stanford Seismic Data?

Symposium - International Astronomical Union
doi 10.1017/s0074180900157857
Full Text
Open PDF
Abstract

Available in full text

Date

January 1, 1988

Authors
A. N. EllisD. O. Gough
Publisher

Cambridge University Press (CUP)


Related search

New Contribution to Scattering of Weakly Interacting Massive Particles on Nuclei

Physical Review Letters
AstronomyPhysics
2003English

Weakly Interacting Massive Particle WIMP

English

Dark Matter of Weakly Interacting Massive Particles and the QCD Equation of State

Physical Review D
2005English

Jeans Instability of Interstellar Gas Clouds in the Background of Weakly Interacting Massive Particles

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
1998English

Superparamagnetic Relaxation of Weakly Interacting Particles

Physical Review Letters
AstronomyPhysics
1994English

Aspects of the Gluonic Production of Weakly Interacting Particles

1989English

Weakly Interacting Massive Particle Distribution in and Evaporation From the Sun

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
1987English

Limits on Spin-Independent Interactions of Weakly Interacting Massive Particles With Nucleons From the Two-Tower Run of the Cryogenic Dark Matter Search

Physical Review Letters
AstronomyPhysics
2006English

Seismic Tests for Solar Models With Tachocline Mixing

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2002English

Amanote Research

Note-taking for researchers

Follow Amanote

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

Privacy PolicyRefund Policy