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相关论文: Seismic Search for Strange Quark Nuggets

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A precise characterisation of the red giants in the seismology fields of the CoRoT satellite is a prerequisite for further in-depth seismic modelling. The optical spectra obtained for 19 targets have been used to accurately estimate their…

It has been suggested to use seismic detectors on the Moon as a tool to search for gravitational waves in an intermediate frequency range between mHz and Hz. Employing three different spherically symmetric models for the lunar interior, we…

广义相对论与量子宇宙学 · 物理学 2024-08-26 M. Kachelriess , M. P. Nødtvedt

Free neutrons have a measured lifetime of 880 s, but disagreement between existing laboratory measurements of ~10 s have persisted over many years. This uncertainty has implications for multiple physics disciplines, including standard-model…

核实验 · 物理学 2020-12-30 David J. Lawrence , Jack T. Wilson , Patrick N. Peplowski

We discuss the possible appearance of strange exotic multi-quark states in the interior of neutron stars and signals for the existence of strange quark matter in the core of compact stars. We show how the in-medium properties of possible…

天体物理学 · 物理学 2009-11-11 Irina Sagert , Mirjam Wietoska , Jurgen Schaffner-Bielich

The possibility to determine the axial strange form factor of the nucleon from neutrino scattering experiments is studied. The existing experimental information is reviewed and several related observables which could be measured in the near…

高能物理 - 唯象学 · 物理学 2007-05-23 W. M. Alberico , C. Maieron

Antiquark nuggets are hypothetical compact composite objects conjectured to account for a significant fraction of dark matter in the Universe. In contrast to quark nuggets, these objects consist of antimatter. They may remain undetected if…

高能物理 - 唯象学 · 物理学 2025-01-13 V. V. Flambaum , I. B. Samsonov , G. K. Vong

Strange quark matter with the density of ~ 5\times 10^{14} g cm^{-3} might exist up to the surface of a strange star. This differs qualitatively from the case of a neutron star and opens observational possibilities to distinguish strange…

天体物理学 · 物理学 2007-05-23 Vladimir V. Usov

An overview of hints for new physics outside the Standard Model and the status of sparticle and Higgs searches is given. The present limits on Higgs bosons of about 90 GeV as well as the $\bsg$ rate and cosmological constraints severely…

高能物理 - 唯象学 · 物理学 2009-09-25 W. de Boer

Quasi-periodic oscillations (QPOs) have been discovered in the X-ray emission of many neutron stars and black holes. The QPOs with frequencies greater than about 300 Hz are thought to be produced near the surfaces of neutron stars and the…

天体物理学 · 物理学 2009-06-23 Frederick K. Lamb

The Moon provides a huge effective detector volume for ultrahigh energy cosmic neutrinos, which generate coherent radio pulses in the lunar surface layer due to the Askaryan effect. In light of presently considered lunar missions, we…

天体物理学 · 物理学 2008-11-26 O. Stål , J. E. S. Bergman , B. Thidé , L. K. S. Daldorff , G. Ingelman

The strange quark matter (SQM) may be the ground state of QCD; nuggets of SQM could be present in cosmic rays (CR). SLIM is a large area experiment, using CR39 and Makrofol track etch detectors, presently deployed at the high altitude CR…

高能物理 - 实验 · 物理学 2015-07-21 S. Balestra , S. Cecchini , G. Giacomelli , R. Giacomelli , M. Giorgini , S. Manzoor , L. Patrizii , V. Popa , O. Saavedra

In dark matter axion searches, quantum uncertainty manifests as a fundamental noise source, limiting the measurement of the quadrature observables used for detection. We use vacuum squeezing to circumvent the quantum limit in a search for a…

Near-Earth supernova blasts which engulf the solar system have left traces of their ejecta in the geological and lunar records. There is now a wealth of data on live radioactive ${}^{60}$Fe pointing to a supernova at 3 Myr ago, as well as…

太阳与恒星天体物理 · 物理学 2023-09-22 Adrienne F. Ertel , Brian D. Fields

With the recent findings from various astrophysical results hinting towards possible existence of strange quark matters with the baryonic resonances such as $\Lambda^0, \Sigma^0, \Xi, \Omega$ in the core of neutron stars, we investigate the…

高能物理 - 唯象学 · 物理学 2022-08-18 Hiranmaya Mishra , Prasanta K. Panigrahi , Sudhanwa Patra , Utpal Sarkar

We study the structure and total energy of a strange quark star (SQS) endowed with a strong magnetic field with different rotational frequencies. The MIT bag model is used, with the density-dependent bag constant for the equation of state…

高能天体物理现象 · 物理学 2023-05-08 Fatemeh Kayanikhoo , Mateusz Kapusta , Miljenko Čemeljić

Prepared for Snowmass 2013 e-Proceedings. We review a testable dark matter model outside of the standard WIMP paradigm in which the observed ratio Omega_{dark} ~ 5 Omega_{visible} for visible and dark matter densities finds its natural…

宇宙学与河外天体物理 · 物理学 2013-09-13 Kyle Lawson , Ariel R. Zhitnitsky

We investigate the possibility to use the neutrinos coming from a future galactic supernova explosion to perform neutrino oscillation tomography of the Earth's core. We propose to use existing or planned detectors, resulting in an…

高能物理 - 唯象学 · 物理学 2014-11-17 Manfred Lindner , Tommy Ohlsson , Ricard Tomas , Walter Winter

The possibility off measuring for the first time neutrino-nuclei coherent scattering has been recently discussed by several experimental collaborations. It is shown that such a measurement may be very sensitive to non-standard interactions…

高能物理 - 唯象学 · 物理学 2009-11-11 J. Barranco , O. G. Miranda , T. I. Rashba

I describe the current status of the solar neutrino problem, summarizing the arguments that its resolution will require new particle physics. The phenomenon of matter-enhanced neutrino oscillations is reviewed. I consider the implications…

核理论 · 物理学 2007-05-23 W. C. Haxton

The cosmic first order phase transition from quarks to hadrons, occurring a few microseconds after the Big Bang, would lead to the formation of quark nuggets which would be stable on a cosmological time scale, if the associated baryon…

天体物理学 · 物理学 2011-02-11 Jan-e Alam , Sibaji Raha , Bikash Sinha
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