Ghisellini 2007 火球与静止物质的膨胀产生伽玛暴
主要内容:
提出了标准内激波模型的一些弊端:效率要求不同shell的Lorentz因子相差很大,早期余辉的变平,Amati等统计关系不能从标准模型推出。然后提出在暴源不远的外边可能存在一个静止的物质块,火球与它撞上产生了伽玛暴。
精彩摘抄:
文章信息:
- arXiv:0709.1945 [ps, pdf, other]
- Title: Re-born fireballs in Gamma-Ray BurstsAuthors: G. Ghisellini (1), A. Celotti (2), G. Ghirlanda (1), C. Firmani (1,3), L. Nava (1,4) ((1) INAF-Oss. Astr. di Brera, (2) SISSA, Trieste, (3) U.N.A.M., Mexico, (4) Univ. Insubria)Comments: 5 pages, 3 Figures, accepted for publication in MNRAS (Letters)Subjects: Astrophysics (astro-ph)
We consider the interaction between a relativistic fireball and material assumed to be still located just outside the progenitor star. Only a small fraction of the expected mass is sufficient to efficiently decelerate the fireball, leading to dissipation of most of its kinetic energy. Since the scattering optical depths are still large at distances comparable to the progenitor radius, the dissipated energy is trapped in the system, accelerating it to relativistic velocities. The process resembles the birth of another fireball at radii R~1e11 cm, not far from the transparency radius, and with a starting bulk Lorentz factors Gamma_c~10. As seen in the observer frame, this "re--generated" fireball appears collimated within an angle theta_j=1/Gamma_c. If the central engine works intermittently, the funnel can, at least partially, refill and the process can repeat itself. We discuss how this idea can help solving some open issues of the more conventional internal shock scenario for interpreting the Gamma-Ray Burst properties.
Labels: 1.2 non-standard model, 1.e efficiency
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