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The late infall of cold dark matter onto an isolated galaxy such as our own produces flows with definite velocity vectors at any physical point in the galactic halo. It also produces caustics which are places where the dark matter density…

天体物理学 · 物理学 2016-11-03 P. Sikivie , W. Kinney

The late infall of cold dark matter onto our galaxy produces discrete flows and caustics in its halo. The recently discovered ring of stars near galactocentric distance 20 kpc and a series of sharp rises in the Milky Way rotation curve are…

天体物理学 · 物理学 2014-10-13 Pierre Sikivie

Axion physics is briefly reviewed. Constraints from laboratory searches, astrophysics and cosmology require the axion mass to be in the range $10^{-6} \lesssim m_a < 3\cdot 10^{-3}$eV. Near the lower end of this range, axions are all or a…

高能物理 - 唯象学 · 物理学 2017-08-23 P. Sikivie

The late infall of cold dark matter onto an isolated galaxy produces flows with definite local velocity vectors throughout the galactic halo. It also produces caustic rings, which are places in the halo where the dark matter density is very…

天体物理学 · 物理学 2009-10-31 P. Sikivie

We present a proposal for the full phase space distribution of the Milky Way halo. The model is axially and reflection symmetric and its time evolution is self-similar. It describes the halo as a set of discrete dark matter flows with…

天体物理学 · 物理学 2009-02-20 L. D. Duffy , P. Sikivie

We simulate the growth of isolated dark matter haloes from self-similar and spherically symmetric initial conditions. Our N-body code integrates the geodesic deviation equation in order to track the streams and caustics associated with…

宇宙学与河外天体物理 · 物理学 2015-05-13 Mark Vogelsberger , Simon D. M. White , Roya Mohayaee , Volker Springel

We test a particular theory of dark matter in which dark matter axions form ring "caustics" in the plane of the Milky Way against actual observations of Milky Way stars. According to this theory, cold, collisionless dark matter particles…

We show that most particle and subhalo orbits in simulated cosmological cold dark matter halos are surprisingly regular and periodic: The phase space structure of the outer halo regions shares some of the properties of the classical…

天体物理学 · 物理学 2009-11-13 J. Diemand , M. Kuhlen

I investigate the caustics produced by the fall of collisionless dark matter in and out of a galaxy in the limit of negligible velocity dispersion. The outer caustics are spherical shells enveloping the galaxy. The inner caustics are rings.…

天体物理学 · 物理学 2009-10-31 P. Sikivie

The late infall of dark matter onto a galaxy produces structure (such as caustics) in the distribution of dark matter in the halo. We argue that such structure is likely to occur generically on length scales proportional to $l \sim t_0…

天体物理学 · 物理学 2009-10-31 William H. Kinney , Pierre Sikivie

Although a simple argument implies that the distribution of dark matter in galactic halos is characterized by discrete flows and caustics, their presence is often ignored in discussions of galactic dynamics and of dark matter detection…

天体物理学 · 物理学 2008-11-26 Aravind Natarajan , Pierre Sikivie

State-of-the-art hydrodynamical simulations show that gas inflow through the virial sphere of dark matter halos is focused (i.e. has a preferred inflow direction), consistent (i.e. its orientation is steady in time) and amplified (i.e. the…

宇宙学与河外天体物理 · 物理学 2015-05-28 C. Pichon , D. Pogosyan , T. Kimm , A. Slyz , J. Devriendt , Y. Dubois

We use cosmological simulations of isolated Milky Way-mass galaxies, as well as Local Group analogues, to define the "edge" -- a caustic manifested in a drop in density or radial velocity -- of Galactic-sized haloes, both in dark matter and…

We prove that a flow of cold collisionless particles from all directions in and out of a region necessarily forms a caustic. A corollary is that, in cold dark matter cosmology, galactic halos have inner caustics in addition to the more…

天体物理学 · 物理学 2009-11-13 Aravind Natarajan , Pierre Sikivie

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…

天体物理学 · 物理学 2009-05-22 V. Onemli , P. Sikivie

It is shown that the infall of collisionless dark matter onto isolated galaxies produces a series of caustic rings in the halo dark matter distribution. The properties of these caustics are investigated. The density profile of the caustic…

天体物理学 · 物理学 2009-10-30 Pierre Sikivie

An all high-latitude sky survey for cool carbon giant stars in the Galactic halo has revealed 75 such stars, of which the majority are new detections. Of these, more than half are clustered on a Great Circle on the sky which intersects the…

天体物理学 · 物理学 2009-10-31 Rodrigo Ibata , Geraint F. Lewis , Michael Irwin , Edward Totten , Thomas Quinn

From the scale-free nature of gravity, the structure in the universe is expected to be self-similar on large scales. However, this self-similarity will eventually break down due to small-scale gas physics such as star formation, AGN and…

宇宙学与河外天体物理 · 物理学 2025-09-17 Benjamin A. Seidel , Rhea-Silvia Remus , Lucas M. Valenzuela , Lucas C. Kimmig , Klaus Dolag

The Gaia map of the Milky Way reveals a pair of triangular features at nearly symmetric locations on opposite sides of the Galactic Center. In this paper we explore the implications of these features assuming they are manifestations of a…

星系天体物理 · 物理学 2021-06-10 Sankha S. Chakrabarty , Yaqi Han , Anthony H. Gonzalez , Pierre Sikivie

The recently discovered ring of stars near Galactocentric distance $r = 20$ kpc is interpreted as baryonic matter accreted onto the second caustic ring of dark matter in our galaxy. Caustic rings of dark matter were predicted in the…

天体物理学 · 物理学 2007-05-23 Pierre Sikivie
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