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> Index of every page on this site: [llms.txt](https://index.cbpf.br/llms.txt)

**Nota de Física****Publicado**

# **Weak-Scale Hidden Sector and Energy Transport in Fireball Models of Gamma-Ray Bursts**

**Durmus A. Demir; Herman J. Mosquera Cuesta**

2000

[**Descargar PDF **0,1 MB](https://index.cbpf.br/files/publicacao/6ad2a767639f62b11adbb3eb/pdf) [**Contactar al responsable**](mailto:apub@cbpf.br?subject=Weak-Scale%20Hidden%20Sector%20and%20Energy%20Transport%20in%20Fireball%20Models%20of%20Gamma-Ray%20Bursts)

## **Datos de la publicación**

<dl>

<dt>Autores</dt>
<dd>Durmus A. Demir; Herman J. Mosquera Cuesta</dd>

<dt>Tipo</dt>
<dd>Nota de Física</dd>

<dt>Estado</dt>
<dd>Publicado</dd>

<dt>Fecha de publicación</dt>
<dd>2000</dd>

<dt>Descripción</dt>
<dd>The annihilation of pairs of very weakly interacting particles in the neibourghood of gamma-ray sources is introduced here as a plausible mechanism to overcome the baryon load problem. This way we can explain how these very high energy gamma-ray bursts can be powered at the onset of very energetic events like supernovae (collapsars) explosions or coalescences of binary neutron stars. Our approach uses the weak-scale hidden sector models in which the Higgs sector of the standard model is extended to include a gauge singlet that only interacts with the Higgs particle. These particles would be produced either during the implosion of the red supergiant star core or at the aftermath of a neutron star binary merger. The whole energetics and timescales of the relativistic blast wave, the fireball, are reproduced.</dd>

<dt>Año</dt>
<dd>2000</dd>

<dt>Número</dt>
<dd>CBPF-NF-079/00</dd>

<dt>Vínculo con tesis</dt>
<dd>No</dd>

<dt>Vínculo con beca</dt>
<dd>No</dd>

</dl>

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```

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