Constraints on finite-range baryonic and leptonic forces from stellar evolution

J. A. Grifols; E. Massó

doi:10.1016/0370-2693(86)90509-5

Constraints on finite-range baryonic and leptonic forces from stellar evolution

J. A. Grifols, E. Massó

Departament de Física

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The contribution to stellar energy loss is considered that would result if finite-range baryonic and.or leptonic forces exist. By requiring that these new interactions do not upset standard models on stellar evolution dynamics upper limits are placed on their strengths. In particular, α E <4×10 -26 is found from solar data and α E <4×10 -28 from data on red giants for the fine structure constant α E of a force coupled to the electronic number. © 1986.

Idioma original	Anglès
Pàgines (de-a)	237-240
Revista	Physics Letters B
Volum	173
DOIs	https://doi.org/10.1016/0370-2693(86)90509-5
Estat de la publicació	Publicada - 12 de juny 1986

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10.1016/0370-2693(86)90509-5

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title = "Constraints on finite-range baryonic and leptonic forces from stellar evolution",

abstract = "The contribution to stellar energy loss is considered that would result if finite-range baryonic and.or leptonic forces exist. By requiring that these new interactions do not upset standard models on stellar evolution dynamics upper limits are placed on their strengths. In particular, α E <4×10 -26 is found from solar data and α E <4×10 -28 from data on red giants for the fine structure constant α E of a force coupled to the electronic number. {\textcopyright} 1986.",

author = "Grifols, {J. A.} and E. Mass{\'o}",

year = "1986",

month = jun,

day = "12",

doi = "10.1016/0370-2693(86)90509-5",

language = "English",

volume = "173",

pages = "237--240",

journal = "Physics Letters B",

issn = "0370-2693",

publisher = "Elsevier",

}

TY - JOUR

T1 - Constraints on finite-range baryonic and leptonic forces from stellar evolution

AU - Grifols, J. A.

AU - Massó, E.

PY - 1986/6/12

Y1 - 1986/6/12

N2 - The contribution to stellar energy loss is considered that would result if finite-range baryonic and.or leptonic forces exist. By requiring that these new interactions do not upset standard models on stellar evolution dynamics upper limits are placed on their strengths. In particular, α E <4×10 -26 is found from solar data and α E <4×10 -28 from data on red giants for the fine structure constant α E of a force coupled to the electronic number. © 1986.

AB - The contribution to stellar energy loss is considered that would result if finite-range baryonic and.or leptonic forces exist. By requiring that these new interactions do not upset standard models on stellar evolution dynamics upper limits are placed on their strengths. In particular, α E <4×10 -26 is found from solar data and α E <4×10 -28 from data on red giants for the fine structure constant α E of a force coupled to the electronic number. © 1986.

U2 - 10.1016/0370-2693(86)90509-5

DO - 10.1016/0370-2693(86)90509-5

M3 - Article

SN - 0370-2693

VL - 173

SP - 237

EP - 240

JO - Physics Letters B

JF - Physics Letters B

ER -

Constraints on finite-range baryonic and leptonic forces from stellar evolution

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