Radiation from matter-antimatter annihilation in the quark nugget model of dark matter
نویسندگان
چکیده
We revisit the properties of positron cloud in quark nugget (QN) model dark matter (DM). In this model, particles are represented by compact composite objects composed a large number quarks or antiquarks with total baryon $B\sim 10^{24}$. These have very small density our galaxy which makes them "dark" to all DM detection experiments and cosmological observations. scenario, anti-quark nuggets play special role because they may manifest themselves annihilation visible matter. study electron-positron collisions free electrons, hydrogen helium gases nuggets. show that strong electric field destroys positronium, atoms prevents electrons from penetrating deeply cloud, thus reducing probability nearly five orders magnitude. Therefore, electron QNs cannot explain observed SPI/INTEGRAL detector photons energy 511 keV center galaxy. be explained different mechanism QN captures protons annihilate anti-quarks core transform neutrons charge increasing temperature. As result loses positrons space there. Even more produced charged pions resulting proton annihilation. Another manifestation emission $\pi^0$ decays.
منابع مشابه
Antimatter from supersymmetric dark matter
We propose low–energy antideuterons in cosmic rays as a new possible signature for indirect detection of supersymmetric dark matter. Since the energy spectrum of the antiproton secondary component is still spoilt by considerable theoretical uncertainties, looking for low–energy antideuterons seems a plausible alternative. We apply our calculation to the AMS experiment, when mounted on the Inter...
متن کاملDark matter spikes and annihilation radiation from the galactic center.
The annihilation rate of weakly interacting cold dark matter particles at the galactic center could be greatly enhanced by the growth of a density spike around the central supermassive black hole (SBH). Here we discuss the effects of hierarchical mergers on the central spike. Mergers between halos containing SBHs lead to the formation of SBH binaries which transfer energy to the dark matter par...
متن کاملExtragalactic gamma-ray background radiation from dark matter annihilation
If dark matter is composed of neutralinos, one of the most exciting prospects for its detection lies in observations of the gamma-ray radiation created in pair annihilations between neutralinos, a process that may contribute significantly to the extragalactic gamma-ray background (EGB) radiation. We here use the high-resolution MillenniumII simulation of cosmic structure formation to produce th...
متن کاملAnnihilation Radiation of Dark Matter in Heterotic Orbifold Models
Gianfranco Bertone 1, Pierre Binétruy 2,3, Yann Mambrini 4, Emmanuel Nezri 2,3 1 NASA/Fermilab Astrophysics Group, Fermi National Accelerator Laboratory, Box 500 Batavia, IL 60510-0500 2 Laboratoire de Physique Théorique des Hautes Energies, Université Paris-Sud, F-91405 Orsay 3 APC Université Paris 7, Collège de France, F-75231 Paris Cedex 05 and 4 Departamento de F́ısica Teórica C-XI and Insti...
متن کاملAntimatter Signatures of Gravitino Dark Matter Decay
The scenario of gravitino dark matter with broken R-parity naturally reconciles three paradigms that, albeit very well motivated separately, seem to be in mutual conflict: supersymmetric dark matter, thermal leptogenesis and standard Big Bang nucleosynthesis. Interestingly enough, the products of the gravitino decay could be observed, opening the possibility of indirect detection of gravitino d...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
ژورنال
عنوان ژورنال: Physical review
سال: 2021
ISSN: ['0556-2813', '1538-4497', '1089-490X']
DOI: https://doi.org/10.1103/physrevd.104.063042