Photinos from gravitational collapse

J. A. Grifols; E. Massó; S. Peris

doi:10.1016/0370-2693(89)90792-2

Photinos from gravitational collapse

J. A. Grifols, E. Massó, S. Peris

Departamento de Física

Producción científica: Contribución a una revista › Artículo › Investigación › revisión exhaustiva

24 Citas (Scopus)

Resumen

Very light photinos, if they exist, should be produced in a SN explosion. Using the data from SN 1987A we set limits on the masses of selectrons (and squarks), the SUSY particles involved in the production (and diffusion) of photinos in the stellar medium. The bounds obtained are m e ̃>75 GeV (250 GeV) form q ̃>45 GeV (80 GeV), where m e ̃≡m e ̃L=m e ̃R. © 1989.

Idioma original	Inglés
Páginas (desde-hasta)	591-596
Publicación	Physics Letters B
Volumen	220
DOI	https://doi.org/10.1016/0370-2693(89)90792-2
Estado	Publicada - 13 abr 1989

Acceder al documento

10.1016/0370-2693(89)90792-2

Otros archivos y enlaces

https://www.scopus.com/pages/publications/0041383366

Citar esto

@article{403c896bf42046b8a96b014f33703432,

title = "Photinos from gravitational collapse",

abstract = "Very light photinos, if they exist, should be produced in a SN explosion. Using the data from SN 1987A we set limits on the masses of selectrons (and squarks), the SUSY particles involved in the production (and diffusion) of photinos in the stellar medium. The bounds obtained are m e{\~ }>75 GeV (250 GeV) form q{\~ }>45 GeV (80 GeV), where m e{\~ }≡m e{\~ }L=m e{\~ }R. {\textcopyright} 1989.",

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

year = "1989",

month = apr,

day = "13",

doi = "10.1016/0370-2693(89)90792-2",

language = "English",

volume = "220",

pages = "591--596",

journal = "Physics Letters B",

issn = "0370-2693",

publisher = "Elsevier",

}

TY - JOUR

T1 - Photinos from gravitational collapse

AU - Grifols, J. A.

AU - Massó, E.

AU - Peris, S.

PY - 1989/4/13

Y1 - 1989/4/13

N2 - Very light photinos, if they exist, should be produced in a SN explosion. Using the data from SN 1987A we set limits on the masses of selectrons (and squarks), the SUSY particles involved in the production (and diffusion) of photinos in the stellar medium. The bounds obtained are m e ̃>75 GeV (250 GeV) form q ̃>45 GeV (80 GeV), where m e ̃≡m e ̃L=m e ̃R. © 1989.

AB - Very light photinos, if they exist, should be produced in a SN explosion. Using the data from SN 1987A we set limits on the masses of selectrons (and squarks), the SUSY particles involved in the production (and diffusion) of photinos in the stellar medium. The bounds obtained are m e ̃>75 GeV (250 GeV) form q ̃>45 GeV (80 GeV), where m e ̃≡m e ̃L=m e ̃R. © 1989.

UR - https://www.scopus.com/pages/publications/0041383366

U2 - 10.1016/0370-2693(89)90792-2

DO - 10.1016/0370-2693(89)90792-2

M3 - Article

SN - 0370-2693

VL - 220

SP - 591

EP - 596

JO - Physics Letters B

JF - Physics Letters B

ER -

Photinos from gravitational collapse

Resumen

Acceder al documento

Otros archivos y enlaces

Huella

Citar esto