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相关论文: Signatures of Mirror Stars

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Non-minimal hidden sectors are an important generic possibility and arise in highly motivated theories like Neutral Naturalness. A fraction of dark matter could therefore have hidden interactions analogous to Standard Matter (SM)…

高能物理 - 唯象学 · 物理学 2020-03-25 David Curtin , Jack Setford

Mirror Stars are a generic prediction of dissipative dark matter models, including minimal atomic dark matter and twin baryons in the Mirror Twin Higgs. Mirror Stars can capture regular matter from the interstellar medium through extremely…

高能天体物理现象 · 物理学 2023-12-01 Isabella Armstrong , Berkin Gurbuz , David Curtin , Christopher Matzner

Mirror Stars are a generic prediction of dissipative dark matter models, including minimal atomic dark matter and twin baryons in the Mirror Twin Higgs. Mirror Stars capture regular atoms from the interstellar medium through highly…

高能天体物理现象 · 物理学 2026-04-02 Franco Cabral , Stuart Williamson , David Curtin , Christopher D. Matzner

The fundamental nature of dark matter is entirely unknown. A compelling candidate is Twin Higgs mirror matter, invisible hidden-sector cousins of the Standard Model particles and forces. This predicts mirror neutron stars made entirely of…

高能天体物理现象 · 物理学 2023-05-12 Maurício Hippert , Jack Setford , Hung Tan , David Curtin , Jacquelyn Noronha-Hostler , Nicolas Yunes

The mirror twin Higgs model is a candidate for (strongly-interacting) complex dark matter, which mirrors SM interactions with heavier quark masses. A consequence of this model are mirror neutron stars -- exotic stars made entirely of mirror…

高能天体物理现象 · 物理学 2023-07-05 Maurício Hippert , Emily Dillingham , Hung Tan , David Curtin , Jacquelyn Noronha-Hostler , Nicolás Yunes

Mirror dark matter, where dark matter resides in a hidden sector exactly isomorphic to the standard model, can be probed via direct detection experiments by both nuclear and electron recoils if the kinetic mixing interaction exists. In…

高能物理 - 唯象学 · 物理学 2017-01-04 J. D. Clarke , R. Foot

The oscillation of the neutron $n$ into mirror neutron $n'$, its partner from dark mirror sector, can gradually transform an ordinary neutron star into a mixed star consisting in part of mirror dark matter. The implications of the reverse…

高能天体物理现象 · 物理学 2021-06-22 Zurab Berezhiani

We suggest that the major fraction of binary mergers, which might provide gravitational wave signal detectable by LIGO/Virgo, emerged from the hidden mirror sector. Mirror particles do not interact with an ordinary observer except…

高能天体物理现象 · 物理学 2020-04-03 Revaz Beradze , Merab Gogberashvili , Alexander S. Sakharov

Given the lack of empirical evidence of weakly interacting dark matter, it is reasonable to look to other candidates such as a confining dark sector with a similar number of particles as the standard model. Twin Higgs mirror matter is one…

Mirror matter is a stable self-collisional dark matter candidate. If exact mirror parity is a conserved symmetry of nature, there could exist a parallel hidden (mirror) sector of the Universe which has the same kind of particles and the…

宇宙学与河外天体物理 · 物理学 2014-11-20 Paolo Ciarcelluti

Asymmetric dark matter under certain conditions could form compact star-like objects, which can be searched either through gravitational lensing or by observation of gravitational waves from binaries involving such compact objects. In this…

高能物理 - 唯象学 · 物理学 2023-10-09 Boris Betancourt Kamenetskaia , Anja Brenner , Alejandro Ibarra , Chris Kouvaris

Mirror matter is a self-collisional dark matter candidate. If exact mirror parity is a conserved symmetry of the nature, there could exist a parallel hidden (mirror) sector of the Universe which has the same kind of particles and the same…

天体物理学 · 物理学 2010-03-16 P. Ciarcelluti

A simple way to accommodate dark matter is to postulate the existence of a hidden sector. That is, a set of new particles and forces interacting with the known particles predominantly via gravity. In general this leads to a large set of…

宇宙学与河外天体物理 · 物理学 2014-05-13 R. Foot

Mirror matter is a stable self-collisional dark matter candidate. If parity is a conserved unbroken symmetry of nature, there could exist a parallel hidden (mirror) sector of the Universe composed of particles with the same masses and…

宇宙学与河外天体物理 · 物理学 2011-03-31 Paolo Ciarcelluti

Mirror symmetry is a plausible candidate for a fundamental symmetry of particle interactions which can be exactly conserved if a set of mirror particles exist. The properties of the mirror particles seem to provide an excellent candidate to…

高能物理 - 唯象学 · 物理学 2008-11-26 R. Foot , S. Mitra

The oscillation of neutrons $n$ into mirror neutrons $n'$, their mass degenerate partners from dark mirror sector, can have interesting implications for neutron stars: an ordinary neutron star could gradually transform into a mixed star…

高能天体物理现象 · 物理学 2021-12-08 Zurab Berezhiani , Riccardo Biondi , Massimo Mannarelli , Francesco Tonelli

Mirror matter is an entirely new form of matter predicted to exist if mirror symmetry is a fundamental symmetry of nature. Mirror matter has the right broad properties to explain the inferred dark matter of the Universe and might also be…

天体物理学 · 物理学 2009-11-07 R. Foot , S. Mitra

The physics of kinetic mixing between ordinary and mirror photons is discussed. An important role is played by four linear combinations we dub the physical photon, the sterile photon, the physical mirror photon, and the sterile mirror…

天体物理学 · 物理学 2008-11-26 R. Foot , A. Yu. Ignatiev , R. R. Volkas

The possibility that mirror matter with masses in the several hundred GeV- TeV range exists is explored. Mirror matter appears quite naturally in many unified models of particle interactions both in GUTs and in strings often in vector-like…

高能物理 - 唯象学 · 物理学 2014-11-20 Tarek Ibrahim , Pran Nath

Dark matter could have a dissipative asymmetric subcomponent in the form of atomic dark matter (aDM). This arises in many scenarios of dark complexity, and is a prediction of neutral naturalness, such as the Mirror Twin Higgs model. We show…

高能物理 - 唯象学 · 物理学 2021-06-25 David Curtin , Jack Setford
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