[PDF] Top 20 Head-on collisions of unequal mass black holes in D=5 dimensions
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Head-on collisions of unequal mass black holes in D=5 dimensions
... Black holes (BHs) have been at the center stage of fundamental physics in the last decades: supermassive, astrophysical BHs lurk at the center of most galaxies while large numbers ... See full document
6
Extra dimensions at the CERN LHC via mini-black holes: Effective Kerr-Newman brane-world effects
... size of extra dimensions, and therefore can be considered as totally embedded in a D-dimensional ...other in LHC, their gravi- tational attraction increases steadily, and they can enter ... See full document
12
Search for microscopic black holes in $pp$ collisions at $\sqrt{s}=7$ TeV
... microscopic black holes in pp collisions at a center-of-mass energy of 7 TeV is ...presence of multiple energetic jets, leptons, and photons, which are typical ... See full document
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Search for black holes and sphalerons in high-multiplicity final states in proton-proton collisions at $ \sqrt{s}=13 $ TeV
... LHC in proton-proton collisions at a center- of-mass energy of 13 TeV in ...regions in data without any reliance on ...limits on the cross section of ... See full document
47
Search for microscopic black holes in pp collisions at sqrt(s) = 8 TeV
... likelihood of the observed number of events, given the predicted background multiplied by the likelihoods of a set of measurements of the nuisance parameters that are related to vari- ... See full document
33
Search for resonances and quantum black holes using dijet mass spectra in proton-proton collisions at $\sqrt{s} =$ 8 TeV
... cube of the resonance mass, like the RS graviton or the color-octet ...dijet mass due to convolution of the tail with PDFs is visible in ...section in the narrow-width ... See full document
45
Head-on collisions and orbital mergers of Proca stars
... solutions of the Einstein-(complex)-Proca ...that of black holes, thus yielding an example of a black hole mimicker, which, moreover, can be both stable and form dynamically from ... See full document
16
Dilatonic black holes in superstring gravity
... follows: in Sec. II, we will solve the dilaton field equation in d dimensions, in the background of a spherically symmetric black hole, in the presence of ... See full document
9
Inside black holes with synchronized hair
... clouds on Kerr, i.e. smoothness on the event horizon and strong oscilla- tions near the Cauchy horizon, should be generic for any test field obeying the synchronization condition (on the event ... See full document
9
Formation of massive seed black holes via collisions and accretion
... form in our simulations, but we only categorize the indi- vidual stellar ...components. In Fig. 3 we present the time evolution of the fraction of protostars belonging to each of these ... See full document
17
Mass inflation in a D-dimensional Reissner-Nordstrom black hole: A hierarchy of particle accelerators?
... charged black holes exhibit mass inflation, quite analogous to their four dimensional counterparts (see [ 24 ] for a recent study of lower dimensional black ...charged black hole ... See full document
8
Search for narrow resonances and quantum black holes in inclusive and $b$-tagged dijet mass spectra from $pp$ collisions at $\sqrt{s}=7$ TeV
... resulting in a broader di- jet mass shape and, consequently, weaker expected ...depend on whether the 0 and 1 b-tag mass shapes are dominated by gluons or quarks in the final ...sets ... See full document
37
Black holes in a box: Toward the numerical evolution of black holes in AdS space-times
... case of asymptotically flat space- times, a BH binary under the influence of a reflective shell does not settle down into a stationary configuration soon after ...state of the system manifests itself ... See full document
17
Search for black holes in high-multiplicity final states in proton-proton collisions at $ \sqrt{s}=$13 TeV
... physics in energetic, high-multiplicity final states has been performed using proton– proton collision data collected with the CMS detector at a center-of-mass energy of 13 TeV and ... See full document
29
Numerical Relativity in D dimensional space-times: Collisions of unequal mass black holes
... simulations in we refer the reader to Table 1 in [15]. The mass parameters of the smaller BH are given by r D−3 S,1 /r D−3 S = ...values of the second BH are adapted ... See full document
5
Black ringoids: spinning balanced black objects in d >= 5 dimensions - the codimension-two case
... follows: in the next section we present a discussion of the coordinate system used to impose a non-spherical topology of the event ...introduced in section 3. In section 4 we review the ... See full document
50
An analytic effective model for hairy black holes
... Hairy black holes (BHs) have macroscopic degrees of freedom which are not associated with a Gauss ...degrees of freedom are not manifest as quasi-local quantities computed at the ...Based ... See full document
7
Collisions in primordial star clusters: formation pathway for intermediate mass black holes
... given in Fig. 3, showing the fraction of collisions as a function of stellar radius and for di fferent num- bers of ...reliability of the results. We find that the total fraction ... See full document
9
Stationary Black Holes and Light Rings
... shadow of the astrophysically significant Kerr black hole (BH) are both intimately connected to a special set of bound null orbits known as light rings ...orbits? In this Letter we prove the ... See full document
5
Shadows of Kerr Black Holes with Scalar Hair
... prospect of testing one of its most dramatic consequences: black holes ...existence of event horizons, the defining property of ...channel of observation —gravitational ... See full document
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