Rapid publication: manuscripts are peer-reviewed and a first decision provided to authors approximately 20 days after submission; acceptance to publication is undertaken in 5 days.

Recognition of reviewers: reviewers who provide timely, thorough peer-review reports receive vouchers entitling them to a discount on the APC of their next publication in any SCIREA journal, in appreciation of the work done.

Archiving

Volume 5, Issue 2, April 2023

Open Access

Could the number of blue straggler stars help to determine the age of their parent globular cluster?

Félix Llorente de Andrés

Abstract: A recent study shows, from an empirical deduction, that the number and the presence of the blue straggler stars (BSS) in an open cluster follow a function whose components are the ratio between age and the relaxation time, ƒ, and a factor, ϖ, which is an indicator of stellar collisions plus primordial binaries. The relation

Abstract References PDF (511 k) 89 Downloads 93093 Views DOI: 10.54647/astronomy160048

Volume 5, Issue 1, February 2023

Open Access

Basis on Negative Matter as Unified Dark Matter and Dark Energy

Yi-Fang Chang

Abstract: Based on Dirac negative energy, Einstein mass-energy relation and principle of equivalence, we propose the negative matter as the simplest model of unified dark matter and dark energy. All theories are known, only mass includes positive and negative. Because there is repulsion between positive matter and negative matter, so

Abstract References PDF (333 k) 76 Downloads 87525 Views DOI: 10.54647/astronomy160043

Open Access

Ultrasonic technology of detection of gravitational waves of neutron stars - pulsars

Chernobay Ivan Alesandrovich

Abstract: The work relates to the creation of new methods and instruments for observational astronomy, in particular to gravitational astrophysics. The ultrasonic gravitational method for obtaining information about such exotic objects as neutron pulsar stars has been developed and successfully tested. Gravitational waves are detecte

Abstract References PDF (686 k) 86 Downloads 87432 Views DOI: 10.54647/astronomy160044

Volume 4, Issue 1, February 2022

Open Access

ON THE ORIGIN OF MOON AND CONTINENTS

Flavio Barbiero

Abstract: All astronomical bodies originate inside clouds of gas and dust, therefore there should be a common process that leads to their condensation. A galactic cloud normally has some turbulence and therefore a gradient of speeds from point to point. Thanks to it, a vortex originates that rakes the material of the surrounding clou

Abstract References PDF (526 k) 94 Downloads 87878 Views DOI: 10.54647/astronomy16035

Open Access

DARK MATTER – TRANSVERSE MASS

Flavio Barbiero

Abstract: The dark matter is a mysterious kind of matter with no mass, no inertia and none of the other characteristics that we attribute to matter, but for the fact that it exerts a force that prevents the stars of the arms of the spiral galaxies to disperse into space. A force that, to achieve this result, should decrease not with

Abstract References PDF (1299 k) 87 Downloads 87644 Views DOI: 10.54647/astronomy16039

Volume 3, Issue 2, April 2019

Open Access

Conjecture on the Origin of the Solar System

Liu Taixiang

Abstract: This paper briefly describes the principle of the formation of the solar system, and explains the cause of the Titius-Bode law, the rotational angular momentum and revolutionary momentum of a celestial body.

Abstract References PDF (412 k) 240 Downloads 89251 Views DOI:

Volume 3, Issue 1, February 2019

Open Access

Implications of detecting the Axion-Like Particles in Astro-Particle Physics

K K Singh

Abstract: Axions and axion like particles in general are consequences of the extensions of the standard model in particle physics. Axions have been proposed as hypothetical pseudo-scalar particles in particle physics to solve the strong Charge-Parity problem using quantum chromodynamics. These particles are also proposed to be an att

Abstract References PDF (186 k) 341 Downloads 113045 Views DOI:

Open Access

Universe's challenges: What is next?

Peter Kopanov

Abstract: In this paper we consider a quantitative relationship between the probabilistic standard normal distribution and the distribution of matter and energy in the Universe, according to the observations from the Planck cosmic laboratory.

Abstract References PDF (223 k) 279 Downloads 113299 Views DOI:

Volume 2, Issue 2, August 2018

Open Access

SOME CHARACTERISTICS OF COSMIC MICROWAVE BACKROUND RADIATION

Michał Marek

Abstract: Data gathered by the Planck i.e. maps of temperature Cosmic Microwave Background (CMB) have been used for analysis of a number of counts of the CMB as a function of their temperature by IDL software. Recently I presented a histogram made by Fv software (Marek 2018). Power-law slope for reasonable range of data is alpha=1.81.

Abstract References PDF (147 k) 1465 Downloads 113944 Views DOI:

Volume 2, Issue 1, June 2018

Open Access

IS THE UNIVERSE A SELF-ORGANIZED CRITICALITY SYSTEM?

Michał Marek

Abstract: Sandpile Paradigm was proposed by Bak, Tang and Wiesenfeld (Bak et al. 1987) to explain simple model of Self-Organized Criticality (SOC). When the piles fall on the sandpile (input driver), we will see, that at some critical point (reaching adequate angle of response), sand will slide down to get the saturation phase.
T

Abstract References PDF (610 k) 283 Downloads 113475 Views DOI:

Volume 1, Issue 1, April 2017

Open Access

A proposed new gravitational redshift function to the theoretical model of Morris-Thorne wormholes

Raul Isea

Abstract: This work introduces a new gravitational redshift function to the Morris-Thorne wormhole model that is defined as Φ(r)≡r_0/r ln⁡(r/r_0 ) with spherical symmetry and stabilized by phantom energy.

Abstract References PDF (384 k) 331 Downloads 7748 Views DOI: