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Related papers: Effects of a dark matter caustic passing through t…

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We looked at the orbital motions of test particles according to the External Field Effect (EFE) predicted by the MOdified Newtonian Dynamics (MOND) in the Oort cloud which falls in the deep MONDian regime (r\approx 50-150 kAU). Concerning…

General Relativity and Quantum Cosmology · Physics 2014-11-20 Lorenzo Iorio

We interpret the recent gravitational lensing observations of Jee et al. \cite{Jee} as first evidence for a {\it caustic} ring of dark matter in a galaxy cluster. A caustic ring unavoidably forms when a cold collisionless flow falls with…

Astrophysics · Physics 2009-05-22 V. Onemli , P. Sikivie

We study the solar emission of light dark sector particles that self-interact strongly enough to self-thermalize. The resulting outflow behaves like a fluid which accelerates under its own thermal pressure to highly relativistic bulk…

High Energy Physics - Phenomenology · Physics 2022-11-21 Jae Hyeok Chang , David E. Kaplan , Surjeet Rajendran , Harikrishnan Ramani , Erwin H. Tanin

The solar system's Zodiacal Cloud is visible to the unaided eye, yet the origin of its constituent dust particles is not well understood, with a wide range of proposed divisions between sources in the asteroid belt and Jupiter Family…

Comets have been invoked in numerous studies as a potentially important source of dust and gas around stars, but none has studied the thermo-physical evolution, out-gassing rate, and dust ejection of these objects in such stellar systems.…

Earth and Planetary Astrophysics · Physics 2016-04-14 Ulysse Marboeuf , Amy Bonsor , Jean-Charles Augereau

Within the dark matter paradigm, explaining observed orbital dynamics at galactic level through the inclusion of a dominant dark halo, implies also the necessary appearance of dynamical friction effects. Satellite galaxies, globular…

Astrophysics of Galaxies · Physics 2019-02-28 X. Hernandez

We point out a new and largely model-independent constraint on the dark matter scattering cross section with nucleons, applying when this quantity is larger than for typical weakly interacting dark matter candidates. When the dark matter…

Astrophysics · Physics 2008-11-26 Gregory D. Mack , John F. Beacom , Gianfranco Bertone

We use 7 years of electron and positron Fermi-LAT data to search for a possible excess in the direction of the Sun in the energy range from 42 GeV to 2 TeV. In the absence of a positive signal we derive flux upper limits which we use to…

High Energy Astrophysical Phenomena · Physics 2020-01-15 A. Cuoco , P. De La Torre Luque , F. Gargano , M. Gustafsson , F. Loparco , M. N. Mazziotta , D. Serini

Exocomets are small bodies releasing gas and dust which orbit stars other than the Sun. Their existence was first inferred from the detection of variable absorption features in stellar spectra in the late 1980s using spectroscopy. More…

Dark matter (DM) particles captured by the Sun can produce high energy electrons outside the Sun through annihilating into meta-stable mediators. The corresponding cosmic-ray electron signals observed by the space-based experiments will be…

High Energy Physics - Phenomenology · Physics 2022-04-27 Mohammadreza Zakeri , Yu-Feng Zhou

Cold dark matter particles with an intrinsic matter-antimatter asymmetry do not annihilate after gravitational capture by the Sun and can affect its interior structure. The rate of capture is exponentially enhanced when such particles have…

High Energy Physics - Phenomenology · Physics 2014-11-20 Mads T. Frandsen , Subir Sarkar

With the availability of considerably more data, we revisit the question of how special our Solar System is, compared to observed exoplanetary systems. To this goal, we employ a mathematical transformation that allows for a meaningful,…

Earth and Planetary Astrophysics · Physics 2015-09-16 Rebecca G. Martin , Mario Livio

We study how the classical tests of general relativity are modified by the presence of a subdominant dark matter halo in the solar system. We use a general formalism to calculate the corrected expression for the relevant parameters, and…

General Relativity and Quantum Cosmology · Physics 2012-07-26 Giuseppe De Risi , Tiberiu Harko , Francisco S. N. Lobo

The gravitational action of the smooth energy-matter components filling in the universe can affect the orbit of a planetary system. Changes are related to the acceleration of the cosmological scale size R. In a universe with significant…

Astrophysics · Physics 2008-11-26 M. Sereno , Ph. Jetzer

Impacts by rocky and icy bodies are thought to have played a key role in shaping the composition of solar system objects, including the Earth's habitability. Hence, it is likely that they play a similar role in exoplanetary systems. We…

Earth and Planetary Astrophysics · Physics 2025-02-26 Felix Sainsbury-Martinez , Catherine Walsh , Greg Cooke

Cometary impacts pose a long-term hazard to life on Earth. Impact mitigation techniques have been studied extensively, but they tend to focus on asteroid diversion. Typical asteroid interdiction schemes involve spacecraft physically…

Earth and Planetary Astrophysics · Physics 2019-05-02 Qicheng Zhang , Philip M. Lubin , Gary B. Hughes

(abridged) The Sun's magnetic activity has steadily declined during its main-sequence life. While the solar photospheric luminosity was about 30% lower 4.6 Gyr ago when the Sun arrived on the main sequence compared to present-day levels,…

Astrophysics · Physics 2015-05-13 M. Guedel

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

We present a study of the current state of knowledge concerning spacecraft operations and potential hazards while operating near a comet nucleus. Starting from simple calculations comparing the cometary coma environment to benign conditions…

Earth and Planetary Astrophysics · Physics 2022-04-13 C. M. Lisse , M. R. Combi , T. L. Farnham , N. Dello Russo , S. Sandford , A. F. Cheng , U. Fink , W. M. Harris , J. McMahon , D. J. Scheeres , H. A. Weaver , J. Leary

We numerically investigate the migration of dust particles with initial orbits close to those of the numbered asteroids, observed trans-Neptunian objects, and Comet Encke. The fraction of silicate asteroidal particles that collided with the…

Astrophysics · Physics 2010-12-01 S. I. Ipatov , J. C. Mather , P. A. Taylor
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