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We investigate the possibility for cosmic ray experiments to discover non-thermal small black holes with masses in the TeV range. Such black holes would result due to the impact between ultra high energy cosmic rays or neutrinos with nuclei…

高能物理 - 唯象学 · 物理学 2015-06-04 Xavier Calmet , Lauretiu Ioan Caramete , Octavian Micu

We investigate the possibility to find a characteristic TeV scale quantum black holes decay signature in the data recorded by cosmic rays experiments. TeV black holes can be produced via the collisions of ultra high energetic protons (E >…

高能物理 - 唯象学 · 物理学 2014-07-09 Nicusor Arsene , Lauretiu Ioan Caramete , Peter B. Denton , Octavian Micu

In scenarios with large extra dimensions (LEDs), the fundamental Planck scale can be low enough that collisions between high-energy particles may produce microscopic black holes. High-energy cosmic neutrinos can carry energies much larger…

高能物理 - 唯象学 · 物理学 2020-05-20 Katherine J. Mack , Ningqiang Song , Aaron C. Vincent

It is generally believed that mini black holes decay by emitting elementary particles with a black body energy spectrum. The original calculation lead to the conclusion that about the 90% of the black hole mass is radiated away in the form…

高能物理 - 唯象学 · 物理学 2009-11-11 Alex Casanova , Euro Spallucci

According to recent conjectures on the existence of large extra dimensions in our universe, black holes may be produced during the interaction of Ultra High Energy Cosmic Rays with the atmosphere. However, and so far, the proposed…

高能物理 - 唯象学 · 物理学 2011-05-23 V. Cardoso , M. C. Espirito Santo , M. Paulos , M. Pimenta , B. Tome

The existence of extra degrees of freedom beyond the electroweak scale may allow the formation of black holes in nearly horizontal neutrino air showers. In this paper we examine the average properties of the light descendants of these black…

高能物理 - 唯象学 · 物理学 2009-11-07 Luis Anchordoqui , Haim Goldberg

Ultra-high energy cosmic rays create black holes in scenarios with extra dimensions and TeV-scale gravity. In particular, cosmic neutrinos will produce black holes deep in the atmosphere, initiating quasi-horizontal showers far above the…

高能物理 - 唯象学 · 物理学 2009-07-09 Jonathan L. Feng , Alfred D. Shapere

We consider the production of black holes caused by the collision between high-energy cosmic neutrinos and nuclei contained in detectors. If the fundamental scale M_{*} is O(TEV), as some higher-dimensional theories suggest, ICECUBE…

高能物理 - 唯象学 · 物理学 2009-11-07 Yosuke Uehara

Models with extra dimensions and the fundamental scale at the TeV could imply sign als in large neutrino telescopes due to gravitational scattering of cosmogenic neu trinos in the detection volume. Apart from the production of microscopic…

高能物理 - 唯象学 · 物理学 2007-05-23 J. I. Illana , M. Masip , D. Meloni

If the scale of quantum gravity is near a TeV, the LHC will be producing one black hole (BH) about every second. The BH decays into prompt, hard photons and charged leptons is a clean signature with low background. The absence of…

高能物理 - 唯象学 · 物理学 2008-11-26 Savas Dimopoulos , Greg Landsberg

In the framework of brane-world models lowering the Planck scale to the TeV range, it has recently been pointed out that small black holes could be formed at particle colliders or by neutrinos interactions in the atmosphere. This article…

天体物理学 · 物理学 2008-11-26 A. Barrau , C. Feron , J. Grain

In models with large extra dimensions, where the fundamental gravity scale can be in the electroweak range, gravitational effects in particle physics may be noticeable even at relatively low energies. In this paper, we perform simple…

高能物理 - 唯象学 · 物理学 2008-11-26 C. Bambi , A. D. Dolgov , K. Freese

Thermal relics lighter than an MeV contribute to the energy density of the universe at the time of nucleosynthesis and recombination. Constraints on extra radiation degrees of freedom typically exclude even the simplest of such dark…

高能物理 - 唯象学 · 物理学 2019-05-29 Asher Berlin , Nikita Blinov

We propose an extended version of the standard model, in which neutrino oscillation, dark matter, and baryon asymmetry of the Universe can be simultaneously explained by the TeV-scale physics without assuming unnatural hierarchy among the…

高能物理 - 唯象学 · 物理学 2009-02-27 Mayumi Aoki , Shinya Kanemura , Osamu Seto

We review the perhaps most exciting phenomenology of models with extra spatial dimensions and Planck scale near TeV: the production of mini black holes in ultrahigh energy particle collisions, and the discovery potential of cosmic…

高能物理 - 唯象学 · 物理学 2007-05-23 Huitzu Tu

If spacetime has more than four dimensions, ultra-high energy cosmic rays may create microscopic black holes. Black holes created by cosmic neutrinos in the Earth will evaporate, and the resulting hadronic showers, muons, and taus may be…

高能物理 - 唯象学 · 物理学 2011-05-12 Jaime Alvarez-Muniz , Jonathan L. Feng , Francis Halzen , Tao Han , Dan Hooper

If TeV-scale gravity describes nature, black holes will be produced in particle accelerators, perhaps even with impressive rates at the Large Hadron Collider. Their decays, largely via the Hawking process, will be spectacular. Black holes…

高能物理 - 理论 · 物理学 2016-09-06 Steven B. Giddings

It has been argued that neutrinos originating from ultra-high energy cosmic rays produce black holes deep in the atmosphere in models with TeV-scale quantum gravity. Such black holes would initiate quasi-horizontal showers of particles far…

高能物理 - 唯象学 · 物理学 2008-11-26 Dejan Stojkovic , Glenn D. Starkman , De-Chang Dai

The experimental signatures of TeV-mass black hole (BH) formation in heavy ion collisions at the LHC is examined. We find that the black hole production results in a complete disappearance of all very high $p_T$ ({$> 500$} GeV) back-to-back…

高能物理 - 唯象学 · 物理学 2008-11-26 Horst Stoecker

TeV gravity models provide a scenario for black hole formation at energies much smaller than G_N^(-1/2) \sim 10^19 GeV. In particular, the collision of a ultrahigh energy cosmic ray with a dark matter particle in our galactic halo or with…

高能物理 - 唯象学 · 物理学 2010-02-16 Iacopo Mastromatteo , Petros Draggiotis , Manuel Masip
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