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相关论文: Detecting Planet 9 via Hawking radiation

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Recently, an alleged plausible astrophysical scenario was proposed for the production of observed thermal gamma-ray bursts, via Hawking radiation emitted from a primordial black hole (PBH) freely falling into a more massive black hole. Here…

广义相对论与量子宇宙学 · 物理学 2022-02-08 Tyler McMaken

We evaluate the effects of a distant planet, commonly known as planet 9, on the dynamics of the giant planets of the Solar System. We find that, given the large distance of planet 9, the dynamics of the inner giant planets can be decomposed…

地球与行星天体物理 · 物理学 2016-12-28 Rodney Gomes , Rogerio Deienno , Alessandro Morbidelli

Gravitational microlensing finds planets through their gravitational influence on the light coming from a more distant background star. The presence of the planet is then inferred from the tell-tale brightness variations of the background…

地球与行星天体物理 · 物理学 2018-10-15 Yiannis Tsapras

We study the Hawking radiation from Rotating black holes from gravitational anomalies point of view. First, we show that the scalar field theory near the Kerr black hole horizon can be reduced to the 2-dimensional effective theory. Then,…

高能物理 - 理论 · 物理学 2009-11-11 Keiju Murata , Jiro Soda

In recent years, evidence has been obtained that in the outer region of the Solar System (in the inner part of the Oort cloud), at a distance $\sim300-700$ AU from the Sun, there may be a captured planet or a primordial black hole. In this…

地球与行星天体物理 · 物理学 2024-01-10 Yu. N. Eroshenko , E. A. Popova

The only way to detect planets around stars at distances of several kpc is by (photometric or astrometric) microlensing observations. In this paper, we show that the capability of photometric microlensing extends to the detection of signals…

天体物理学 · 物理学 2007-05-23 G. Covone , R. de Ritis , M. Dominik , A. A. Marino

This paper assesses if the Planet 9 hypothesis, the existence of a ninth planet, is consistent with the planetary hypothesis, the synchronization of sunspot emergence to solar inertial motion (SIM) induced by the planets. We show that SIM…

太阳与恒星天体物理 · 物理学 2022-05-18 Ian R. Edmonds

Are there other planetary systems in our Universe? Indirect evidence has been found for planets orbiting other stars in our galaxy: the gravity of orbiting planets makes the star wobble, and the resulting periodic Doppler shifts have been…

天体物理学 · 物理学 2007-05-23 Edward A. Baltz , Paolo Gondolo

The existence of a hypothetical Planet 9 lurkng in the outer solar system has been invoked as a plausible explanation for the anomalous clustering in the orbits of trans-Neptunian objects. Here we propose that some meteoroids arriving at…

地球与行星天体物理 · 物理学 2023-03-08 Hector Socas-Navarro

Recent analyses of the orbits of some Kuiper Belt objects hypothesize the presence of an undiscovered Neptune-size planet at a very large separation from the Sun. The energy budget of Neptunes on such distant orbits is dominated by the…

地球与行星天体物理 · 物理学 2016-05-04 Sivan Ginzburg , Re'em Sari , Abraham Loeb

The distribution of the orbital elements of the known extreme trans-Neptunian objects or ETNOs has been found to be statistically incompatible with that of an unperturbed asteroid population following heliocentric or, better, barycentric…

地球与行星天体物理 · 物理学 2016-08-23 C. de la Fuente Marcos , R. de la Fuente Marcos

We discuss the feasibility of and present initial designs and approximate cost estimates for a large ($N\sim2000$) network of small photometric telescopes that is purpose-built to monitor $V \lesssim 15$ Gaia Mission program stars for…

地球与行星天体物理 · 物理学 2019-06-26 Malena Rice , Gregory Laughlin

The search for extrasolar Earth-like planets is underway. Over 100 extrasolar giant planets are known to orbit nearby sun-like stars, including several in multiple-planet systems. These planetary systems are stepping stones for the search…

天体物理学 · 物理学 2009-11-07 S. Seager

I review constraints on solar system-bound dark matter, and discuss the possibility that dark matter could be gravitationally bound to the earth and other planets. I briefly survey various empirical constraints on such planet-bound dark…

地球与行星天体物理 · 物理学 2009-04-06 Stephen L. Adler

The Planet Nine hypothesis encompasses a body of about 5-8 Earth's masses whose orbital plane would be inclined to the ecliptic by one or two tens of degrees and whose perihelion distance would be as large as about 240-385 astronomical…

地球与行星天体物理 · 物理学 2026-02-03 Lorenzo Iorio

Gravitational microlensing is known for baryoninc dark matter searches. Here we show that microlensing also provides a unique tool for the detection of low mass planets (such as earths and neptunes) from the ground. A planetary system forms…

天体物理学 · 物理学 2009-10-28 S. H. Rhie , D. P. Bennett

We study the method of calculating the Hawking radiation via gravitational anomalies in gravitational backgrounds of constant negative curvature. We apply the method to topological black holes and also to topological black holes conformally…

高能物理 - 理论 · 物理学 2009-07-24 Eleftherios Papantonopoulos , Petros Skamagoulis

Direct detection of dark matter continues to elude scientists' many attempts to see it interact, and still to this day the only way we know it is there is through observed gravitational effects. The many search experiments are at the point…

高能物理 - 实验 · 物理学 2022-09-29 Nickolas Solomey , Shrey Tripathi

The study of planets beyond the solar system and the search for other habitable planets and life is just beginning. Ground-based (radial velocity and transits) and space-based surveys (transits and astrometry) will identify planets spanning…

The detection of lower mass planets now being reported via radial velocity and microlensing surveys suggests that they may be ubiquitous. If missions such as Kepler are able to confirm this, the detection and study of rocky planets via…

地球与行星天体物理 · 物理学 2009-02-24 Philip M. Hinz , Scott Kenyon , Michael R. Meyer , Alan Boss , Roger Angel