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Most of the matter in the universe is invisible. I review the status of dark matter and describe how both the theory of galaxy formation and novel types of experimental searches are revitalizing attempts to find non-baryonic dark matter.

Astrophysics · Physics 2010-12-09 Joseph Silk

In this work we review some of the theoretical efforts and experimental evidences related to Dark matter and Dark energy problems in the universe. These dilemmas show us how incomplete our knowledge of gravity is, and how our concepts about…

General Relativity and Quantum Cosmology · Physics 2016-05-25 A. J. S. Capistrano , P. I. Odon

We show that Earth mass planets orbiting stars in the Galactic disk and bulge can be detected by monitoring microlensed stars in the Galactic bulge. The star and its planet act as a binary lens which generates a lightcurve which can differ…

Astrophysics · Physics 2011-04-21 David P. Bennett , Sun Hong Rhie

Gravitational lensing studies suggest that the Universe may contain a population of dark galaxies; we investigate this intriguing possibility and propose a mechanism to explain their nature. In this mechanism a dark galaxy is formed with a…

Astrophysics · Physics 2016-01-13 Raul Jimenez , A. F. Heavens , M. R. S. Hawkins , P. Padoan

With no firm evidence for life beyond our solar system, inferences about the population observers such as ourselves rests upon the Earth as a single input, at least for now. Whilst the narrative of our home as a 'humdrum' system has become…

Instrumentation and Methods for Astrophysics · Physics 2025-10-03 David Kipping

Modelling of Extreme Scattering Events suggests that the Galaxy's dark matter is an undetected population of cold, AU-sized, planetary-mass gas clouds. None of the direct observational constraints on this picture -- thermal/non-thermal…

Astrophysics · Physics 2015-06-24 Mark Walker , Mark Wardle

(Abridged) Cosmology faces three distinct challenges in the next decade. (1) The dark sector, both dark matter and dark energy, dominates the Universe. Key questions include determining the nature of both. Improved observational probes are…

Astrophysics · Physics 2007-12-19 Richard Ellis , Joseph Silk

The composition of the dark universe although hypothesised, remains one of the biggest mysteries in modern physics. On smaller scales, there are various solar puzzling phenomena which known physics cannot explain like the coronal heating…

High Energy Physics - Experiment · Physics 2024-04-04 M. Maroudas

Interstellar dust is still a dominant uncertainty in Astronomy, limiting precision in e.g., cosmological distance estimates and models of how light is re-processed within a galaxy. When a foreground galaxy serendipitously overlaps a more…

Astrophysics of Galaxies · Physics 2017-03-29 B. W. Holwerda , W. C. Keel

Genesis Cosmology is the combination of Genesis and a cosmology model for the description of the first three days in Genesis. The first day involves the emergence of the separation of light and darkness from the formless, empty, and dark…

High Energy Physics - Phenomenology · Physics 2011-02-10 Ding-Yu Chung

Naturalness problems such as the hierarchy problem and the origin of dark energy remain significant challenges in modern cosmology. This paper develops a rigorous mathematical framework where each observer defines their own universe, and…

General Relativity and Quantum Cosmology · Physics 2025-05-13 Ruby P. Madeimy

I discuss some of the most outstanding challenges in relativistic astrophysics in the subjects of: compact objects (Black Holes and Neutron Stars); dark sector (Dark Matter and Dark Energy); plasma astrophysics (Origin of Jets, Cosmic Rays…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-15 Reuven Opher

This paper presents an information-theoretic view of how an observer within a quantum system will perceive his world. It is argued that because of the indistinguishability of quantum particles, a coherent state will appear to an observer…

Astrophysics · Physics 2007-05-23 Subhash Kak

The fastest pulsar and the slowest nova; the oldest galaxies and the youngest stars; the weirdest life forms and the commonest dwarfs; the highest energy particles and the lowest energy photons. These were some of the extremes of…

Astrophysics · Physics 2009-11-13 Virginia Trimble , Markus J. Aschwanden , Carl J. Hansen

We present a scenario for galaxy formation based on the hypothesis of scalar field dark matter. We interpret galaxy formation through the collapse of a scalar field fluctuation. We find that a cosh potential for the self-interaction of the…

General Relativity and Quantum Cosmology · Physics 2014-11-17 Miguel Alcubierre , F. Siddhartha Guzman , Tonatiuh Matos , Dario Nunez , L. Arturo Urena-Lopez , Petra Wiederhold

A substantial fraction the stellar mass attributed to galaxies is invisible: stars close to the hydrogen burning limit, brown dwarfs, white dwarfs, neutron stars and black holes. These constituents do, however, gravitationally micro-lens…

Astrophysics of Galaxies · Physics 2017-12-04 Paul L. Schechter

TRAPPIST-1 is a fantastic nearby (~39.14 light years) planetary system made of at least seven transiting terrestrial-size, terrestrial-mass planets all receiving a moderate amount of irradiation. To date, this is the most observationally…

Earth and Planetary Astrophysics · Physics 2020-08-05 Martin Turbet , Emeline Bolmont , Vincent Bourrier , Brice-Olivier Demory , Jérémy Leconte , James Owen , Eric T. Wolf

The naked-eye star 55 Cancri hosts a planetary system with five known planets, including a hot super-Earth (55 Cnc e) extremely close to its star and a farther out giant planet (55 Cnc b), found in milder irradiation conditions with respect…

Despite the recent discoveries of planets orbiting stars at all evolutionary stages, the evolution of planetary systems remains poorly understood. Studying planetary systems around red giant branch stars can reveal how main sequence…

Earth and Planetary Astrophysics · Physics 2024-10-23 Samuel K. Grunblatt

The microlens parallax is a crucial observable for conclusively identifying the nature of lens systems in microlensing events containing or composed of faint (even dark) astronomical objects such as planets, neutron stars, brown dwarfs, and…