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相关论文: The Scalar Hexaquark $uuddss$: a Candidate to Dark…

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It has recently been proposed that the relatively inert, highly symmetric, neutral flavor singlet scalar hadron made of uuddss quarks may have a mass < 2 (m_p + m_e). This is consistent with QCD theory, and with existing accelerator and…

高能物理 - 唯象学 · 物理学 2017-12-01 Glennys R. Farrar

We report on the possibility that the Dark Matter particle is a stable, neutral, as-yet-undiscovered hadron in the standard model. The existence of a compact color-flavor-spin singlet sexaquark (S, uuddss) with mass ~2m_p, is compatible…

高能物理 - 唯象学 · 物理学 2022-01-17 Glennys R. Farrar , Zihui Wang , Xingchen Xu

It is proposed that the neutral, B=2, flavor singlet sexaquark (S) composed of uuddss quarks, has mass m_S <~ 2 GeV. If m_S < 2 (m_p + m_e), it is absolutely stable, while for m_S < m_p+m_e + m_Lambda, its lifetime can be greater than the…

高能物理 - 唯象学 · 物理学 2018-05-11 Glennys R. Farrar

Recent investigations have suggested that the singlet six-quark combination $uuddss$ may be a deeply bound state $S$, called Sexaquark. An essentially stable state $S$ is a potentially excellent Dark Matter candidate. We present the first…

高能物理 - 实验 · 物理学 2020-05-20 Romulus Godang

If dark matter (DM) contains equal numbers of u,d,s quarks, the ratio of DM and ordinary matter densities is shown to follow from the Boltzmann distribution in the Quark Gluon Plasma. For sexaquark DM in the 1860-1880 MeV mass range…

高能物理 - 唯象学 · 物理学 2022-01-17 Glennys R. Farrar

We critically reexamine two possible Dark Matter candidate within the Standard Model. First, we consider the $uuddss$ exa-quark. Its QCD binding energy could be large enough to make it (quasi) stable. We show that the cosmological Dark…

高能物理 - 唯象学 · 物理学 2018-09-19 Christian Gross , Antonello Polosa , Alessandro Strumia , Alfredo Urbano , Wei Xue

Macroscopic nuggets of quark matter were proposed several decades ago as a candidate for dark matter. The formation of these objects in the early universe requires the QCD phase transition to be first order - a requirement that is not…

高能物理 - 唯象学 · 物理学 2018-10-15 Yang Bai , Andrew J. Long

The mass and coupling of the scalar tetraquark $T_{bb;\overline{u}\overline{d }}^{-}$ (hereafter $T_{b:\overline{d}}^{-} $) are calculated in the context of the QCD two-point sum rule method. In computations we take into account effects of…

高能物理 - 唯象学 · 物理学 2020-08-26 S. S. Agaev , K. Azizi , B. Barsbay , H. Sundu

The neutral, flavor singlet scalar uuddss bound state -- the sexaquark, S -- may have a low enough mass to be stable or extremely long-lived. Here we review mass estimates and production expectations and show that laboratory experiments to…

高能物理 - 唯象学 · 物理学 2022-10-20 Glennys R. Farrar

We investigate the possibility that Dark Matter (dm) could be made of scalar candidates and focus, in particular, on the unusual mass range between a few MeV's and a few GeV's. After showing why the Lee-Weinberg limit (which usually forbids…

高能物理 - 唯象学 · 物理学 2009-09-29 C. Boehm , P. Fayet

A color-flavor-spin singlet state of six quarks $uuddss$ ($S$, or sexaquark) has been argued to be a potentially undiscovered deeply bound, long-lived hadron. Theoretical calculations of the $S$ mass have been made in the literature, widely…

高能物理 - 唯象学 · 物理学 2023-09-28 Glennys R. Farrar , Zihui Wang

Recent investigations have suggested that the six-quark combination uuddss could be a deeply bound state (S) that has eluded detection so far, and a potential dark matter candidate. We report the first search for a stable, doubly strange…

高能物理 - 实验 · 物理学 2019-03-06 Bertrand Echenard

The hypothetical $SU(3)$ flavor-singlet dibaryon state $S$ with strangeness $-2$ has been discussed as a dark-matter candidate capable of explaining the curious 5-to-1 ratio of the mass density of dark matter to that of baryons. We study…

高能物理 - 唯象学 · 物理学 2019-03-27 Edward W. Kolb , Michael S. Turner

Dark matter (DM) and neutrinos are the two most compelling pieces of evidence of new physics beyond the Standard Model of Particle Physics but these are often treated as belonging to two different sectors. Yet DM-neutrino interactions are…

高能物理 - 唯象学 · 物理学 2017-05-12 Celine Boehm , Andres Olivares-Del Campo , Sergio Palomares-Ruiz , Silvia Pascoli

If quark matter is energetically favored over nuclear matter at zero temperature and pressure then it has long been expected to take the form of strange quark matter (SQM), with comparable amounts of $u$, $d$, $s$ quarks. The possibility of…

高能物理 - 唯象学 · 物理学 2018-06-06 Bob Holdom , Jing Ren , Chen Zhang

In this paper we study a real scalar field as a possible candidate to explain the dark matter in the universe. In the context of a free scalar field with quadratic potential, we have used Union 2.1 SN Ia observational data jointly with a…

广义相对论与量子宇宙学 · 物理学 2016-08-31 J. F. Jesus , S. H. Pereira , J. L. G. Malatrasi , F. Andrade-Oliveira

We investigate the phenomenology of flavored dark matter (DM). DM stability is guaranteed by an accidental ${\mathcal Z}_3$ symmetry, a subgroup of the standard model (SM) flavor group that is not broken by the SM Yukawa interactions. We…

高能物理 - 唯象学 · 物理学 2016-01-27 Fady Bishara , Admir Greljo , Jernej F. Kamenik , Emmanuel Stamou , Jure Zupan

In the framework of an nonuniversal $U(1)'$ extension of the standard model, we propose an scalar candidate for cold dark matter which exhibits interactions with ordinary matter through Higgs and gauge bosons. Using limits from low energy…

高能物理 - 唯象学 · 物理学 2014-11-07 R. Martinez , J. Nisperuza , F. Ochoa , J. P. Rubio

We construct a scalar dark matter model with $U(1)_{L_\mu-L_\tau}$ symmetry in which the dark matter interacts with the quark flavours, allowing lepton non-universal $b \to s \ell \bar{\ell}$ decays. The model can solve $b \to s \mu \mu$…

高能物理 - 唯象学 · 物理学 2019-11-13 Seungwon Baek

The quantum model of the homogeneous, isotropic, and spatially closed universe predicts an existence of two types of collective quantum states in the universe. The states of one type characterize a gravitational field, the others describe a…

天体物理学 · 物理学 2007-05-23 V. E. Kuzmichev , V. V. Kuzmichev
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