| 查看: 43 | 回复: 0 | |||
[交流]
190、Discrimination on the Origin of 30 PeV Gamma ray Photons
|
|
preprint of cern doi :10.5281/zenodo.21765509 or https://doi.org/10.5281/zenodo.21765509 my academic identifier: orcid id: 0009-0005-2185-5790. you may go to the official academic website to retrieve and view relevant research content. readers may copy this number to search on the official zenodo website (search by english title or english keywords) to view the full english and chinese pdf texts. Abstract At the end of July and early August 2026, the Large High Altitude Air shower Observatory (LHAASO) announced the detection of ultra high energy gamma ray photons up to 30 PeV from the binary system Cygnus X 3, together with periodic variability of this high energy emission. This marks the first identified variable ultra high energy gamma ray source. The observation exceeds the conventional energy limit of approximately 1 PeV for galactic cosmic ray particles and challenges existing astroparticle acceleration theories. The mainstream interpretation attributes the 30 PeV gamma ray emission to secondary radiation produced by proton acceleration and meson decay within black hole jets. Based on the theory of the primacy of light, this paper proposes an alternative physical mechanism: the observed 30 PeV gamma ray photons are primary high energy photons generated by spontaneous energy elevation within the dense photon soup environment inside the black hole, which escape through the accretion disk. Physical inconsistencies within the proton acceleration scenario are analysed and compared with the self consistent photon soup mechanism, providing an alternative approach for understanding the origin of extreme energy astrophysical radiation. Keywords LHAASO observation; 30 PeV gamma ray photon; Cygnus X 3; proton acceleration model; primacy of light theory; photon soup energy rise; hadron dissociation paradox 1. Observable Facts from Public Official Conclusions The observational information adopted in this paper comes from publicly released results of the Institute of High Energy Physics, Chinese Academy of Sciences. The confirmed objective phenomena are listed below: 1.The target of observation is the compact binary system Cygnus X 3, composed of a black hole (or neutron star) and a massive companion star with stable periodic material accretion. 2.Ultra high energy gamma ray photons with energy no less than 30 PeV have been detected, exceeding the traditional galactic particle acceleration energy limit of about 1 PeV. 3.The high energy gamma ray signal shows periodic variation of roughly 4.8 hours, and high energy radiation occurs within a small spatial region surrounding the black hole. 4.This observation proves that radiation sources generating far higher energy levels than conventionally expected exist within the Milky Way galaxy. The above are publicly verifiable observational facts. This paper only discusses the physical mechanism behind radiation generation and does not question the measured observational data itself.  |
回复此楼» 猜你喜欢
厉娜
已经有4人回复
-
售SCI一区T0P文章，我:8.O.55.1.O54,科目全,可伽急
已经有12人回复
-
售SCI-T0P文章，我:8O.5.5.1.O.54,科目齐全,可+急
已经有15人回复
-
售SCI文章，我:8O.5.5.1O.54,科目全,可十急
已经有14人回复
-
售SCI一区T0P文章，我:8O.55.1.O.54,科目全,可伽急
已经有16人回复
-
售SCI文章，我:8O.5.5.1O.54,科目全,可十急
已经有15人回复
-
售SCI一区文章，我:8O5.5.1.O5.4,科目全,可伽急
已经有10人回复
-
售SCI一区T0P文章，我:8O.55.1.O.54,科目全,可伽急
已经有12人回复
-
售SCI一区文章，我:8.O.55.1.O.54,科目齐全,可伽急
已经有8人回复
-
售SCI一区T0P文章，我:8.O.55.1.O.54,科目齐全,可+急
已经有8人回复
