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721por CMS Collaboration“…An update on a search for microscopic black hole production in $pp$ collisions at a center-of-mass energy of 7 TeV by the CMS experiment at the LHC is presented using a 2011 data sample corresponding to an integrated luminosity of 190~pb$^{-1}$. …”
Publicado 2011
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722
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723por CMS Collaboration“…A search for microscopic black hole production in $pp$ collisions at a center-of-mass energy of 7 TeV by the CMS experiment at the LHC is presented using a 2011 data sample corresponding to an integrated luminosity of approximately 1.09~fb$^{-1}$. …”
Publicado 2011
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724por Cantcheff, M.Botta, Gadelha, Alexandre L., Marchioro, Dafni F.Z., Nedel, Daniel Luiz“…Based on Maldacena's description of an eternal AdS-black hole, we reassess the Thermo Field Dynamics (TFD) formalism in the context of the AdS/CFT correspondence. …”
Publicado 2012
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725por CMS Collaboration“…A search for microscopic black holes in pp collisions at a center-of-mass energy of $8$~TeV is presented. …”
Publicado 2012
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726“…This volume covers mainstream topics at research level involving gravitational waves, spinning particles, and black holes suitable for graduates and early postgraduates exploring avenues into research in general relativity.…”
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727
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728por ATLAS, Experiment“…"Black Hole" event superimposed over a classic image of the ATLAS detector.…”
Publicado 2014
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729“…In the first part of the book, we summarize some basic knowledge about black holes and quantum field theory in curved spacetime. …”
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730“…We suggest a proposal of quantization for black holes that is based on an analogy between a black hole and a hydrogen atom. …”
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731
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732
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733
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734
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735
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736“…We propose that Gravitational Wave (GW) bursts with millisecond durations can be explained by the GW emission from the hyperbolic encounters of Primordial Black Holes in dense clusters. These bursts are single events, with the bulk of the released energy happening during the closest approach, and emitted in frequencies within the AdvLIGO sensitivity range. …”
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737por Hektor, Andi, Hütsi, Gert, Marzola, Luca, Raidal, Martti, Vaskonen, Ville, Veermäe, Hardi“…Finally, by imposing that the temperature of the gas at z∼17 does not exceed the indications of EDGES, we constrain the possible abundance of primordial black holes. Depending on uncertainties related to the accretion model, we find that O(10)M⊙ primordial black holes can only contribute to a fraction fPBH<(1–10-3) of the total dark matter abundance.…”
Publicado 2018
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738
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739“…We calculate two- and three-point tachyon amplitudes of the SL(2,R)/U(1) two-dimensional Euclidean black hole for spherical topologies in the continuum approach proposed by Bershadsky and Kutasov. …”
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740