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We investigate if the gamma ray halo, for which recent evidence has been found in EGRET data, can be explained by neutralino annihilations in a clumpy halo. We find that the measured excess gamma ray flux can be explained through a moderate…

天体物理学 · 物理学 2009-10-30 L. Bergstrom , J. Edsjo , P. Ullio

The fundamental question of baryogenesis and the problem of matter-antimatter asymmetry motivate this study into the formation and evolution of antimatter objects in the early Universe. Hypothesize is the existence of isolated antimatter…

高能天体物理现象 · 物理学 2026-02-04 Sattvik Yadav

The Galactic secondary cosmic ray anti-proton flux calculated with different propagation models is fairly consistent with data, and the associated propagation uncertainty is small. This is not the case for any anti-proton exotic component…

天体物理学 · 物理学 2007-05-23 D. Maurin , R. Taillet , C. Combet

The possibility of natural and abundant creation of antimatter in the Universe in a SUSY-baryogenesis model with a scalar field condensate is described. This scenario predicts vast quantities of antimatter, corresponding to galaxy and…

天体物理学 · 物理学 2007-05-23 D. Kirilova , M. Panayotova , T. Valchanov

Cosmic-ray antideuterons could be a key for the discovery of exotic phenomena in our Galaxy, such as dark-matter annihilations or primordial black hole evaporation. Unfortunately the theoretical predictions of the antideuteron flux at Earth…

We carry out a detailed analysis of fluxes of cosmic ray antiprotons, positrons, electrons and photons to be expected from the annihilation of relic heavy neutrinos in the galactic halo. The spectra of particles are evaluated by Monte Carlo…

高能物理 - 唯象学 · 物理学 2007-05-23 Yu. A. Golubkov , R. V. Konoplich

A new generation of upcoming space-based experiments will soon start to probe the spectrum of cosmic ray antiparticles with an unprecedented accuracy and, in particular, will open up a window to energies much higher than those accessible so…

天体物理学 · 物理学 2008-11-26 Torsten Bringmann , Pierre Salati

We estimate the flux of cosmic-ray antiprotons expected from the annihilation of neutralinos in the galactic halo. The antiproton signal may offer an important alternative detection scheme in the case that neutralino annihilation proceeds…

天体物理学 · 物理学 2010-11-30 Gerard Jungman , Marc Kamionkowski

We address the issue of the cosmological bias between matter and galaxy distributions, looking at dark-matter haloes as a first step to characterize galaxy clustering. Starting from the linear density field at high redshift, we follow the…

宇宙学与河外天体物理 · 物理学 2015-05-20 Anna Elia , Suchita Kulkarni , Cristiano Porciani , Massimo Pietroni , Sabino Matarrese

Recent observations of a large excess of cosmic-ray positrons at high energies have raised a lot of interest in leptonic decay modes of dark matter particles. Nevertheless, dark matter particles in the Milky Way halo could also decay…

高能物理 - 唯象学 · 物理学 2009-11-19 Alejandro Ibarra , David Tran

We review gamma-ray observations that constrain antimatter - both baryonic and leptonic - in the Universe. Antimatter can be probed through ordinary matter, with the resulting annihilation gamma-rays providing indirect evidence for its…

高能天体物理现象 · 物理学 2014-01-29 Peter von Ballmoos

Recent observations by the Alpha Magnetic Spectrometer (AMS-02) have tentatively detected a handful of cosmic-ray antihelium events. Such events have long been considered as smoking-gun evidence for new physics, because astrophysical…

高能物理 - 唯象学 · 物理学 2021-03-17 Martin Wolfgang Winkler , Tim Linden

In the present paper we discuss a generation of large antimatter regions with sizes exceeding the critical surviving size. In the modern epoch domains with high antimatter density evolve to single galaxies with a peculiar content of…

宇宙学与河外天体物理 · 物理学 2015-08-07 A. V. Grobov , S. G. Rubin

All galaxies are thought to reside within large halos of dark matter, whose properties can only be determined from indirect observations. The formation and assembly of galaxies is determined from the interplay between these dark matter…

天体物理学 · 物理学 2011-02-11 Lee R. Spitler , Duncan A. Forbes

We use the constraints on the diffusion parameters as obtained with stable nuclei to calculate the cosmic antiproton flux from annihilating relic neutralinos. We discuss the relevance of each characteristic parameter, describing our two…

天体物理学 · 物理学 2007-05-23 Fiorenza Donato , Nicolao Fornengo , David Maurin , Pierre Salati , Richard Taillet

The oscillation of the neutron $n$ into mirror neutron $n'$, its partner from dark mirror sector, can gradually transform an ordinary neutron star into a mixed star consisting in part of mirror dark matter. The implications of the reverse…

高能天体物理现象 · 物理学 2021-06-22 Zurab Berezhiani

In our Galaxy, light antinuclei composed of antiprotons and antineutrons can be produced through high-energy cosmic-ray collisions with the interstellar medium or could also originate from the annihilation of dark-matter particles that have…

核实验 · 物理学 2022-12-19 ALICE Collaboration

Cosmological models which predict a large amount of antimatter in the Universe are reviewed. Observational signatures and searches for cosmic antimatter are briefly considered. A short discussion of new long range forces which might be…

高能物理 - 唯象学 · 物理学 2009-10-22 A. Dolgov

We discuss the hypotheses that cosmological baryon asymmetry and entropy were produced in the early Universe by phase transition of the scalar fields in the framework of spontaneous baryogenesis scenario. We show that annihilation of the…

天体物理学 · 物理学 2009-11-10 Pavel D. Naselsky , Lung-Yih Chiang

Possible existence of antimatter in our Galaxy, in particular of antistars is discussed and the mechanism of their creation is described.

宇宙学与河外天体物理 · 物理学 2022-09-21 A. D. Dolgov