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Related papers: Exotic Decays of Strangelets

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We re-analyze the predictions of chiral-soliton models for the masses and decay widths of baryons in the exotic antidecuplet of flavour SU(3). The calculated ranges of the chiral-soliton moment of inertia and the \pi-nucleon scattering…

High Energy Physics - Phenomenology · Physics 2009-11-10 John Ellis , Marek Karliner , Michal Praszalowicz

The amount of decaying dark matter, accumulated in the central regions in neutron stars together with the energy deposition rate from decays, may set a limit on the neutron star survival rate against transitions to more compact objects…

Solar and Stellar Astrophysics · Physics 2015-04-09 M. Angeles Perez-Garcia , J. Silk

We investigate the stability of strange quark matter and the properties of the corresponding strange stars, within a wide range of quark mass scaling. The calculation shows that the resulting maximum mass always lies between 1.5 solor mass…

Solar and Stellar Astrophysics · Physics 2013-05-15 Ang Li , Ren-Xin Xu , Ju-Fu Lu

Forty years ago Witten suggested that dark matter could be composed of macroscopic clusters of strange quark matter. This idea was very popular for several years, but it dropped out of fashion once lattice QCD calculations indicated that…

High Energy Physics - Phenomenology · Physics 2025-02-19 Francesco Di Clemente , Marco Casolino , Alessandro Drago , Massimiliano Lattanzi , Claudia Ratti

We analyze the conventional perturbative treatment of sphaleron-induced baryon number washout relevant for electroweak baryogenesis and show that it is not gauge-independent due to the failure of consistently implementing the Nielsen…

High Energy Physics - Phenomenology · Physics 2015-12-01 Hiren H. Patel , Michael J. Ramsey-Musolf

As a baryon number violating process with $\Delta B=2$, neutron-antineutron oscillation ($n\to\bar n$) provides a unique test of baryon number conservation. We have performed a search for $n\to\bar n$ oscillation with bound neutrons in…

High Energy Physics - Experiment · Physics 2021-01-27 Kamiokande Collaboration , K. Abe , C. Bronner , Y. Hayato , M. Ikeda , S. Imaizumi , H. Ito , J. Kameda , Y. Kataoka , M. Miura , S. Moriyama , Y. Nagao , M. Nakahata , Y. Nakajima , S. Nakayama , T. Okada , K. Okamoto , A. Orii , G. Pronost , H. Sekiya , M. Shiozawa , Y. Sonoda , Y. Suzuki , A. Takeda , Y. Takemoto , A. Takenaka , H. Tanaka , T. Yano , R. Akutsu , S. Han , T. Kajita , K. Okumura , T. Tashiro , R. Wang , J. Xia , D. Bravo-Berguño , L. Labarga , Ll. Marti , B. Zaldivar , F. d. M. Blaszczyk , E. Kearns , J. D. Gustafson , J. L. Raaf , J. L. Stone , L. Wan , T. Wester , J. Bian , N. J. Griskevich , W. R. Kropp , S. Locke , S. Mine , M. B. Smy , H. W. Sobel , V. Takhistov , P. Weatherly , J. Hill , J. Y. Kim , I. T. Lim , R. G. Park , B. Bodur , K. Scholberg , C. W. Walter , A. Coffani , O. Drapier , S. El Hedri , A. Giampaolo , M. Gonin , Th. A. Mueller , P. Paganini , B. Quilain , T. Ishizuka , T. Nakamura , J. S. Jang , J. G. Learned , L. H. V. Anthony , A. A. Sztuc , Y. Uchida , V. Berardi , M. G. Catanesi , E. Radicioni , N. F. Calabria , L. N. Machado , G. De Rosa , G. Collazuol , F. Iacob , M. Lamoureux , N. Ospina , L. Ludovici , Y. Nishimura , S. Cao , M. Friend , T. Hasegawa , T. Ishida , T. Kobayashi , T. Matsubara , T. Nakadaira , M. Jakkapu , K. Nakamura , Y. Oyama , K. Sakashita , T. Sekiguchi , T. Tsukamoto , Y. Nakano , T. Shiozawa , A. T. Suzuki , Y. Takeuchi , S. Yamamoto , A. Ali , Y. Ashida , J. Feng , S. Hirota , A. K. Ichikawa , T. Kikawa , M. Mori , T. Nakaya , R. A. Wendell , K. Yasutome , P. Fernandez , N. McCauley , P. Mehta , A. Pritchard , K. M. Tsui , Y. Fukuda , Y. Itow , H. Menjo , T. Niwa , K. Sato , M. Tsukada , P. Mijakowski , M. Posiadala-Zezula , C. K. Jung , C. Vilela , M. J. Wilking , C. Yanagisawa , M. Harada , K. Hagiwara , T. Horai , H. Ishino , S. Ito , Y. Koshio , W. Ma , N. Piplani , S. Sakai , Y. Kuno , G. Barr , D. Barrow , L. Cook , A. Goldsack , S. Samani , C. Simpson , D. Wark , F. Nova , T. Boschi , F. Di Lodovico , S. Molina Sedgwick , M. Taani , S. Zsoldos , J. Y. Yang , S. J. Jenkins , J. M. McElwee , M. D. Thiesse , L. F. Thompson , M. Malek , O. Stone , H. Okazawa , S. B. Kim , I. Yu , K. Nishijima , M. Koshiba , N. Ogawa , K. Iwamoto , M. Yokoyama , K. Martens , M. R. Vagins , M. Kuze , S. Izumiyama , M. Tanaka , T. Yoshida , M. Inomoto , M. Ishitsuka , R. Matsumoto , K. Ohta , M. Shinoki , J. F. Martin , H. A. Tanaka , T. Towstego , M. Hartz , A. Konaka , P. de Perio , N. W. Prouse , B. W. Pointon , S. Chen , B. D. Xu , B. Richards , B. Jamieson , J. Walker , A. Minamino , K. Okamoto , G. Pintaudi , R. Sasaki

We study baryon-number-violating processes, including proton and bound neutron decays and $n-\bar n$ oscillations, in a left-right-symmetric (LRS) model in which quarks and leptons have localized wavefunctions in extra dimensions. In this…

High Energy Physics - Phenomenology · Physics 2020-05-14 Sudhakantha Girmohanta , Robert Shrock

It is possible that the proton is stable while atomic hydrogen is not. This is the case in models with new particles carrying baryon number which are light enough to be stable themselves but heavy enough so that proton decay is…

High Energy Physics - Phenomenology · Physics 2020-03-06 David McKeen , Maxim Pospelov

In the large $N_c$ limit both heavy and light baryons are described by the universal mean field, which allows us to relate the properties of heavy baryons to light ones. With the only input from the decays of light octet baryons (due to the…

High Energy Physics - Phenomenology · Physics 2017-12-04 Hyun-Chul Kim , Maxim V. Polyakov , Michal Praszalowicz , Ghil-Seok Yang

We discuss the mass spectrum and strong decays of baryon resonances belonging to the N, Delta, Sigma, Lambda, Xi and Omega families in a collective string-like model for the nucleon. We find good overall agreement with the available data.…

Nuclear Theory · Physics 2017-11-03 R. Bijker , A. Leviatan

We calculate the N_c dependence of the decay widths of exotic eikosiheptaplet within the framework of Chral Quark Soliton Model. We also discuss generalizations of regular baryon representations for arbitrary N_c.

High Energy Physics - Phenomenology · Physics 2008-11-26 Karolina Piesciuk , Michal Praszalowicz

We show that the Standard Model Lagrangian, including small neutrino masses, has an anomaly-free discrete Z_6 symmetry. This symmetry can emerge naturally from I^{3}_{R}+L_i+L_j-2L_k gauge symmetry (L_i is the i-th lepton number) and ensure…

High Energy Physics - Phenomenology · Physics 2009-11-10 K. S. Babu , Ilia Gogoladze , Kai Wang

The role of zero mode quantum corrections to the energy of baryonic systems with exotic quantum numbers (strangeness) is discussed. A simple expression for the contribution depending on strange inertia is obtained in the $SU(3)-$collective…

Nuclear Theory · Physics 2016-01-26 Vladimir Kopeliovich

From a systematic analysis of the energy-dependence of four antibaryon-to-baryon ratios relative to the antikaon-to-kaon ratio, we propose an alternative approach determining the strange-quark chemical potential ($\mu_{\mathrm{s}}$). It is…

High Energy Physics - Phenomenology · Physics 2017-08-03 Abdel Nasser Tawfik , Magda Abdel Wahab , Hayam Yassin , Eman R. Abo Elyazeed , Hadeer M. Nasr El Din

The last decades brought an impressive progress in synthesizing and studying properties of nuclides located very far from the beta stability line. Among the most fundamental properties of such exotic nuclides, usually established first, is…

Nuclear Experiment · Physics 2015-06-03 M. Pfützner , L. V. Grigorenko , M. Karny , K. Riisager

Strange quark matter in beta equilibrium at high densities is studied in a quark confinement model. Two equations of state are dynamically generated for the {\it same} set of model parameters used to describe the nucleon: one corresponds to…

Astrophysics · Physics 2008-11-26 M. Malheiro , M. Fiolhais , A. R. Taurines

Accretion of interstellar material by a magnetized, slowly rotating isolated neutron star is discussed. We show that the average persistent X-ray luminosity of these objects is unlikely to exceed 4x10^26 erg/s. They can also appear as X-ray…

Astrophysics · Physics 2007-05-23 N. R. Ikhsanov , P. L. Biermann

The stability of magnetized strange quark matter (MSQM) is investigated within the phenomenological MIT bag model, taking into account the variation of the relevant input parameters, namely, the strange quark mass, baryon density, magnetic…

Astrophysics · Physics 2010-03-19 R. Gonzalez Felipe , A. Perez Martinez

When considering strangelets at finite temperature it is important to obey the constraint that any observed state must be color singlet. This constraint results in an increase in strangelet masses as calculated at fixed entropy per baryon.…

High Energy Physics - Phenomenology · Physics 2007-05-23 Dan Mønster Jensen , Jes Madsen , Michael B. Christiansen

I make the first estimates of maximum elastic quadrupole deformations sustainable by alternatives to conventional neutron stars. Solid strange quark stars might sustain maximum ellipticities (dimensionless quadrupoles) up to a few times…

Astrophysics · Physics 2007-05-23 Benjamin J. Owen
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