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相关论文: Hawking evaporation of cosmogenic black holes in T…

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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

In models with ``large'' and/or warped extra dimensions, the higher-dimensional Planck scale may be as low as a TeV. In that case black holes with masses of a few TeV are expected to be produced copiously in multi-TeV collisions, in…

高能物理 - 唯象学 · 物理学 2009-11-11 Christian Alig , Manuel Drees , Kin-ya Oda

If gravity becomes strong at the TeV scale, we may have the chance to produce black holes at particle colliders. In this paper we study some experimental signatures of black hole production in TeV-gravity theories. In contrast with the…

高能物理 - 唯象学 · 物理学 2009-11-10 Marco Cavaglia

The production of Large Extra Dimension (LXD) Black Holes (BHs), with a new, fundamental mass scale of $M_f = 1$ TeV, has been predicted to occur at the Large Hadron Collider, LHC, with the formidable rate of $10^8$ per year in p-p…

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

We address the issue of modelling quantum gravity effects in the evaporation of higher dimensional black holes in order to go beyond the usual semi-classical approximation. After reviewing the existing six families of quantum gravity…

高能物理 - 唯象学 · 物理学 2015-05-30 Piero Nicolini , Elizabeth Winstanley

If the scale of quantum gravity is near a TeV, black holes will be copiously produced at the LHC. In this work we study the main properties of the light descendants of these black holes. We show that the emitted partons are closely spaced…

高能物理 - 唯象学 · 物理学 2008-11-26 Luis Anchordoqui , Haim Goldberg

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

If the scale of quantum gravity is near a TeV, the LHC will be producing one black hole (BH) about every second, thus qualifying as a BH factory. With the Hawking temperature of a few hundred GeV, these rapidly evaporating BHs may produce…

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

Models with extra spatial dimensions and TeV-scale gravity offer the first opportunity to test the conjecture of black hole formation in trans-Planckian energy scattering with small impact parameters. After a brief review of gravitational…

高能物理 - 唯象学 · 物理学 2009-11-07 Huitzu Tu

Hawking's groundbreaking prediction that black holes emit thermal radiation and ultimately evaporate remains unverified due to the extreme faintness of this radiation for stellar-mass or larger black holes. In this study, we explore a novel…

高能天体物理现象 · 物理学 2025-09-23 Atreya Acharyya , Giacomo Cacciapaglia , Manuel Meyer , Francesco Sannino

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

TeV scale gravity scenario predicts that the black hole production dominates over all other interactions above the scale and that the Large Hadron Collider will be a black hole factory. Such higher dimensional black holes mainly decay into…

高能物理 - 理论 · 物理学 2009-11-11 Daisuke Ida , Kin-ya Oda , Seong Chan Park

We examine experimental signatures of TeV-mass black hole formation in heavy ion collisions at the LHC. 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 2007-05-23 B. Betz , M. Bleicher , U. Harbach , T. Humanic , B. Koch , H. Stöcker

We study the Hawking evaporation of a class of black hole solutions in dRGT massive gravity, in which the graviton mass gives rise to an effective negative cosmological constant. We found that the effective emission surface can be either…

高能物理 - 理论 · 物理学 2020-12-30 Meng-Shi Hou , Hao Xu , Yen Chin Ong

Black holes could be produced at the Large Hadron Collider in TeV-scale gravity scenarios. We discuss missing energy mechanisms in black hole production and decay in large extra-dimensional models. In particular, we examine how graviton…

高能物理 - 唯象学 · 物理学 2014-11-18 Douglas M. Gingrich

The generalized uncertainty principle, motivated by string theory and non-commutative quantum mechanics, suggests significant modifications to the Hawking temperature and evaporation process of black holes. For extra-dimensional gravity…

高能物理 - 唯象学 · 物理学 2009-11-10 Marco Cavaglia , Saurya Das , Roy Maartens

In theories with large extra dimension and with low quantum gravity scale near a TeV, it is expected that TeV-scale black holes to be produced in proton-proton collisions at the LHC with the center of mass energy of 14 TeV. Since the black…

高能物理 - 唯象学 · 物理学 2009-01-06 M. Mohammadi Najafabadi , S. Paktinat Mehdiabadi

The spectra of gravitational waves from black hole evaporation generically peak at frequencies of order the Hawking temperature, making this signal ultra-high frequency for primordial black holes evaporating in the early universe. This…

广义相对论与量子宇宙学 · 物理学 2024-08-26 Aurora Ireland , Stefano Profumo , Jordan Scharnhorst

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

We study modifications of the Hawking emission in the evaporation of miniature black holes possibly produced in accelerators when their mass approaches the fundamental scale of gravity, set to 1 TeV according to some extra dimension models.…

高能物理 - 唯象学 · 物理学 2007-05-23 G. L. Alberghi , R. Casadio , D. Galli , D. Gregori , A. Tronconi , V. Vagnoni
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