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Related papers: Cosmic balloons

200 papers

Gas rich sub-galactic halos with mass Mt <= 10^7.5 Msun, while incapable of forming stars due to lack of adequate coolants, contain a large fraction of baryonic mass at cosmological reionization. We show that the reionization of the…

Astrophysics · Physics 2009-11-06 Renyue Cen

We calculate energy spectra and mass composition of cosmic rays accelerated by the galactic population of pulsars during their radio and gamma-ray phase. Several models proposed for the distribution of the initial parameters of the galactic…

Astrophysics · Physics 2009-11-10 W. Bednarek , M. Bartosik

Cosmological models in which dark matter consists of cold elementary particles predict that the dark halo population should extend to masses many orders of magnitude below those at which galaxies can form. Here we report a cosmological…

Cosmology and Nongalactic Astrophysics · Physics 2020-09-23 Jie Wang , Sownak Bose , Carlos S. Frenk , Liang Gao , Adrian Jenkins , Volker Springel , Simon D. M. White

Recent observations provide compelling evidence that the bulk of the high energy cosmic rays (CRs) and gamma-ray bursts (GRBs) are co-produced by highly relativistic jets of plasmoids of stellar matter. These jets are launched by fall back…

High Energy Astrophysical Phenomena · Physics 2024-02-06 Shlomo Dado , Arnon Dar

Cosmic-ray energy densities in central regions of starburst galaxies, as inferred from radio and gamma-ray measurements of, respectively, non-thermal synchrotron and neutral pion decay emission, are typically U_p = O(100)eV/cm3, i.e.…

High Energy Astrophysical Phenomena · Physics 2014-11-20 Massimo Persic , Yoel Rephaeli

It is generally believed that cosmological Gamma Ray Bursts (GRBs) are produced by the deceleration of relativistic objects with Lorentz factor (Gamma) >~ 100. We study the possibility that some GRBs are produced along with relativistic…

Astrophysics · Physics 2016-08-30 Hideyuki Umeda

The angular power spectrum and polarization of the cosmic microwave background radiation (CMB), the relative abundances of primordial hydrogen, deuterium and helium isotopes, and the large-scale structure of the universe all indicate that…

Cosmology and Nongalactic Astrophysics · Physics 2011-02-02 Ehud Behar , Shlomo Dado , Arnon Dar , Ari Laor

After a hundred years of searching for the origin of cosmic rays, where and how they are made has finally become clear. Here we briefly trace that odyssey through both astronomical observations and cosmic ray measurements.

High Energy Astrophysical Phenomena · Physics 2015-06-11 Richard E. Lingenfelter

We propose a simple model in which the cosmological dark matter consists of particles whose mass increases with the scale factor of the universe. The particle mass is generated by the expectation value of a scalar field which does not have…

Astrophysics · Physics 2016-10-26 Greg W. Anderson , Sean M. Carroll

The Cold Dark Matter (CDM) hypothesis accurately predicts large-scale structure formation and fits the Cosmic Microwave Background temperature fluctuations (CMB). However, observations of the inner regions of dark matter halos and dwarf…

High Energy Physics - Theory · Physics 2025-02-04 Susobhan Mandal , S. Shankaranarayanan

Super-bubbles are shells in the interstellar medium produced by the simultaneous explosions of many supernova remnants. The solutions of the mathematical diffusion and of the Fourier expansion in 1D, 2D and 3D were deduced in order to…

Astrophysics · Physics 2011-09-20 Lorenzo Zaninetti

We consider the model of a false vacuum bubble with a thin wall where the surface energy density is composed of two different components, "domain-wall" type and "dust" type, with opposite signs. We find stably oscillating solutions, which…

General Relativity and Quantum Cosmology · Physics 2014-11-18 Eduardo I. Guendelman , Nobuyuki Sakai

Our universe has multiple examples of unexplained gravitational losses in black holes and neutron stars. The smallest black holes of about 4 solar masses means the maximum baryon density \rho \approx 10^{17} grams/cm^3. Any collapse of the…

Astrophysics · Physics 2025-05-02 David E. Rosenberg

The most recent observational evidence seems to indicate that giant molecular clouds are predominantly gravitationally unbound objects. In this paper we show that this is a natural consequence of a scenario in which cloud-cloud collisions…

Astrophysics of Galaxies · Physics 2015-05-27 C. L. Dobbs , A. Burkert , J. E. Pringle

Cosmological domain walls can be formed as a result of symmetry breaking at any epoch during the evolution of our universe. We study their interaction with a classical macroscopic object, like Earth or a satellite in Earth's orbit. We set…

General Relativity and Quantum Cosmology · Physics 2022-05-24 De-Chang Dai , Djordje Minic , Dejan Stojkovic

If spacetime torsion couples to the intrinsic spin of matter according to the Einstein-Cartan-Sciama-Kibble theory of gravity, then the resulting gravitational repulsion at supranuclear densities prevents the formation of singularities in…

Cosmology and Nongalactic Astrophysics · Physics 2011-10-26 Nikodem J. Poplawski

The origin of the ultra high energy cosmic rays via annihilation of heavy stable, fermions "f", of the cosmological dark matter (DM) is studied. The particles in question are supposed to be created by the scalaron decays in $R^2$ modified…

High Energy Physics - Phenomenology · Physics 2024-05-22 E. V. Arbuzova , A. D. Dolgov , A. A. Nikitenko

If massive black holes constitute the dark matter in the halo surrounding the Milky Way, the existence of low mass globular clusters in the halo suggests an upper limit to their mass, $M_{_{BH}}$. We use a combination of the impulse…

Astrophysics · Physics 2009-10-22 Ben Moore

We introduce the hypothesis that the matter content of the universe can be a product of the decay of primordial vector bosons. The effect of the intensive cosmological creation of these primordial vector $W, ~Z $ bosons from the vacuum is…

High Energy Physics - Theory · Physics 2016-09-06 D. Blaschke , V. Pervushin , D. Proskurin , S. Vinitsky , A. Gusev

In almost any scenario for 'cosmological' gamma-ray bursts (and in many models where they originate in our own Galaxy), the initial energy density is so large that the resulting relativistic plasma expands with $v\sim c$ producing a blast…

Astrophysics · Physics 2009-10-22 P. Meszaros , M. J. Rees