The Milagro anticenter hot spots: cosmic rays from the Geminga supernova ?
M. Salvati (1), B. Sacco (2) ((1) INAF-Osservatorio di Arcetri,, Firenze, (2) INAF-Istituto di Fisica Cosmica, Palermo)

TL;DR
This paper explores the hypothesis that the TeV cosmic ray excess observed by Milagro near the Geminga supernova remnant originated from that supernova explosion about 340,000 years ago, linking cosmic rays to supernova events.
Contribution
It proposes a novel scenario connecting the Geminga supernova to the observed cosmic ray excess, supported by diffusion models consistent with available data.
Findings
The hypothesis aligns with observed cosmic ray excess data.
Diffusion models (Bohm and free streaming) are consistent with the excess.
Supports supernova origin of cosmic rays in the Milagro region.
Abstract
The Milagro experiment has announced the discovery of an excess flux of TeV cosmic rays from the general direction of the heliotail, also close to the Galactic anticenter. We investigate the hypothesis that the excess cosmic rays were produced in the SN explosion that gave birth to the Geminga pulsar. The assumptions underlying our proposed scenario are that the Geminga supernova occurred about 3.4 10^5 years ago (as indicated by the spin down timescale), that a burst of cosmic rays was injected with total energy 10^49 erg (i.e., about 1% of a typical SN output), and that the Geminga pulsar was born with a positive radial velocity of 100--200 km s^-1. We find that our hypothesis is consistent with the available information. In a first variant (likely oversimplified), the cosmic rays have diffused according to the Bohm prescription (i.e., with a diffusion coefficient on the order of c…
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