中文
相关论文

相关论文: Can Planet 9 be an Axion Star?

200 篇论文

Axions are hypothetical pseudoscalar particles that have been regarded as promising dark matter (DM) candidates. On the other hand, extended compact objects such as axion stars, which are supported by gravity and axion self interactions,…

高能物理 - 唯象学 · 物理学 2025-05-09 Jan Tristram Acuña , Kuan-Yen Chou , Po-Yan Tseng

The axion has emerged in recent years as a leading particle candidate to provide the mysterious dark matter in the cosmos, as we review here for a general scientific audience. We describe first the historical roots of the axion in the…

高能物理 - 唯象学 · 物理学 2022-10-18 Francesca Chadha-Day , John Ellis , David J. E. Marsh

Gas giant planets have been detected on eccentric orbits several hundreds of astronomical units in size around other stars. It has been proposed that even the Sun hosts a wide-orbit planet of 5-10 Earth masses, often called Planet Nine,…

地球与行星天体物理 · 物理学 2025-06-02 André Izidoro , Sean N. Raymond , Nathan A. Kaib , Alessandro Morbidelli , Andrea Isella

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

A hypothetical particle known as the axion holds the potential to resolve both the cosmic dark matter riddle and particle physics' long-standing, strong CP dilemma. An unusually strong 21-cm absorption feature associated with the initial…

高能物理 - 唯象学 · 物理学 2025-10-17 C. R. Das

Axion-photon conversion is a prime mechanism to detect axion-like particles that share a coupling to the photon. We point out that in the vicinity of neutron stars with strong magnetic fields, magnetars, the effective photon mass receives…

高能物理 - 唯象学 · 物理学 2023-10-10 Kyrylo Bondarenko , Alexey Boyarsky , Josef Pradler , Anastasia Sokolenko

We study novel solitonic solutions to Einstein-Klein-Gordon theory in the presence of a periodic scalar potential arising in models of axion-like particles. The potential depends on two parameters: the mass of the scalar field $m_a$ and the…

广义相对论与量子宇宙学 · 物理学 2020-05-27 Davide Guerra , Caio F. B. Macedo , Paolo Pani

Probing the existence of hypothetical particles beyond the Standard model often deals with extreme parameters: large energies, tiny cross-sections, large time scales, etc. Sometimes laboratory experiments can test required regions of…

高能天体物理现象 · 物理学 2021-10-26 P. Tinyakov , M. S. Pshirkov , S. B. Popov

The strong CP problem and its resolution through the existence of an axion are briefly reviewed. The constraints on the axion from accelerator searches, from the evolution of red giants and from supernova SN1987a combine to require $m_a < 3…

高能物理 - 唯象学 · 物理学 2014-11-17 P. Sikivie

Axions may make a significant contribution to the dark matter of the universe. It has been suggested that these dark matter axions may condense into localized clumps, called "axion stars." In this paper we argue that collisions of dilute…

高能物理 - 唯象学 · 物理学 2016-12-09 Stuart Raby

We consider a general class of axion models, including the QCD and string axion, in which the PQ symmetry is broken before or during inflation. Assuming the axion is the dominant component of the dark matter, we discuss axion star formation…

宇宙学与河外天体物理 · 物理学 2020-10-20 Mark P. Hertzberg , Enrico D. Schiappacasse , Tsutomu T. Yanagida

A distant, massive planet in the outer solar system has recently been proposed to explain some observed features of extreme trans-Neptunian objects (TNOs). Here we use N-body simulations of the formation of the Kuiper belt and Oort cloud as…

地球与行星天体物理 · 物理学 2021-10-13 Kalee E. Anderson , Nathan A. Kaib

We show that axion stars formed from axions with nearly Planck-scale decay constants $f$ are unstable to decay, and are unlikely to have phenomenological consequences. More generally, we show how results at smaller $f$ cannot be naively…

高能物理 - 唯象学 · 物理学 2021-06-23 Joshua Eby , Lauren Street , Peter Suranyi , L. C. R. Wijewardhana

We examine high-density axion clusters under gravitational compression. These are transient events in which the majority of axions are rapidly converted into photons, with some configurations producing photon signals with distinctive and…

高能物理 - 唯象学 · 物理学 2025-10-21 Liang Chen , Thomas W. Kephart

We estimate collapse rates of axion stars in our galaxy based on the axion minicluster mass function of the Milky Way dark matter halo. We consider axion-like particles with different temperature evolution of the axion mass, including the…

高能物理 - 唯象学 · 物理学 2024-10-18 Dennis Maseizik , Joshua Eby , Hyeonseok Seong , Günter Sigl

We present novel findings concerning the parameter space of axion stars, extended object forming in dense dark matter environments through gravitational condensation. We emphasize their formation within the dense minihalos that potentially…

高能物理 - 唯象学 · 物理学 2024-10-04 Ziwen Yin , Luca Visinelli

Axion-like dark matter whose symmetry breaking occurs after the end of inflation predicts enhanced primordial density fluctuations at small scales. This leads to dense axion minihalos (or miniclusters) forming early in the history of the…

高能物理 - 唯象学 · 物理学 2023-11-28 Patrick J. Fox , Neal Weiner , Huangyu Xiao

The present surge for the astrophysical relevance of boson stars stems from the speculative possibility that these compact objects could provide a considerable fraction of the non-baryonic part of dark matter within the halo of galaxies.…

广义相对论与量子宇宙学 · 物理学 2009-10-31 Eckehard W. Mielke , Franz E. Schunck

We present a comprehensive study of axion condensed neutron stars that arise in models of an exceptionally light axion that couples to quantum chromodynamics (QCD). These axions solve the strong-charge-parity (CP) problem, but have a…

高能物理 - 唯象学 · 物理学 2025-08-15 Mia Kumamoto , Junwu Huang , Christian Drischler , Masha Baryakhtar , Sanjay Reddy

Most matter in the Universe is invisible and unknown, which is called dark matter. A candidate of dark matter is axion, which is an ultra-light particle motivated as a solution for the CP problem. Axions form clouds in a galactic halo,…

广义相对论与量子宇宙学 · 物理学 2022-10-14 Takuya Tsutsui , Atsushi Nishizawa