2,888 research outputs found
The Beetle Reference Manual: chip version 1.2
This paper details the electrical specifications, operating conditions and port definitions of the readout chip Beetle 1.2. The chip is developed for the LHCb experiment and fulfils the requirements of the silicon vertex detector (VELO, VETO), the silicon tracker and the RICH detector in case of multi-anode photomultiplier readout. It integrates 128 channels with low-noise charge-sensitive preamplifiers and shapers. The pulse shape can be chosen such that it complies with LHCb specifications: a peaking time of 25 ns with a remainder of the peak voltage after 25 ns of less than 30%. A comparator per channel with configurable polarity provides a binary signal. Four adjacent comparator channels are being ORed and brought off chip via LVDS ports. Either the shaper or comparator output is sampled with the LHC-bunch-crossing frequency of 40 MHz into an analog pipeline. This ring buffer has a programmable latency of max. 160 sampling intervals and an integrated derandomising buffer of 16 stages. For analog readout data is multiplexed with up to 40 MHz onto 1 or 4 ports. A binary readout mode operates at up to 80 MHz output rate on two ports. Current drivers bring the serialised data off chip. The chip can accept trigger rates of up to 1.1 MHz to perform a dead-timeless readout within 900 ns per trigger. For te stabi lity and calibration purposes, a charge injector with adjustable pulse height is implemented. The bias settings and various other parameters can be controlled via a standard I2C-interface. Appropriate design measures have been taken to ensure the radiation hardness against total ionising dose effects in excess of 10 Mrad. A robustness against Single Event Upset is achieved by redundant logic
Sub-TeV hadronic interaction model differences and their impact on air showers
In the sub-TeV regime, the most widely used hadronic interaction models
disagree significantly in their predictions of particle spectra from cosmic ray
induced air showers. We investigate the nature and impact of model
uncertainties, focussing on air shower primaries with energies around the
transition between high and low energy hadronic interaction models, where the
dissimilarities are largest and which constitute the bulk of the interactions
in air showers.Comment: Proceedings of the 51 International Symposium on Multiparticle
Dynamics (ISMD2022
Galactic Gamma Halo by Heavy Neutrino annihilations?
The diffused gamma halo around our Galaxy recently discovered by EGRET could
be produced by annihilations of relic neutrinos N (of fourth generation), whose
mass is within a narrow range (Mz /2 < M < Mz). Neutrino annihilations in the
halo may lead to either ultrarelativistic electron pairs whose inverse Compton
Scattering on infrared or optical galactic photons could be the source of the
observed GeV gamma rays, or to prompt 100 MeV- 1 GeV photons (due to neutral
pion secondaries) born by N - anti N --> Z--> quark pairs reactions. The
consequent gamma flux (10 ^(-7)- 10^(-6) cm ^(-2) s^(-1) sr^(-1)) is well
comparable to the EGRET observed one and it is also compatible with the narrow
window of neutrino mass : 45 GeV < M < 50 GeV recently required to explain the
underground DAMA signals. The presence of heavy neutrinos of fourth generation
do not contribute much to solve the dark matter problem of the Universe, but it
may be easily detectable by outcoming LEP II data.Comment: 16 pages, Latex text,in press in Astroparticle Physics 199
Do Evaporating Black Holes Form Photospheres?
Several authors, most notably Heckler, have claimed that the observable
Hawking emission from a microscopic black hole is significantly modified by the
formation of a photosphere around the black hole due to QED or QCD interactions
between the emitted particles. In this paper we analyze these claims and
identify a number of physical and geometrical effects which invalidate these
scenarios. We point out two key problems. First, the interacting particles must
be causally connected to interact, and this condition is satisfied by only a
small fraction of the emitted particles close to the black hole. Second, a
scattered particle requires a distance ~ E/m_e^2 for completing each
bremsstrahlung interaction, with the consequence that it is improbable for
there to be more than one complete bremsstrahlung interaction per particle near
the black hole. These two effects have not been included in previous analyses.
We conclude that the emitted particles do not interact sufficiently to form a
QED photosphere. Similar arguments apply in the QCD case and prevent a QCD
photosphere (chromosphere) from developing when the black hole temperature is
much greater than Lambda_QCD, the threshold for QCD particle emission.
Additional QCD phenomenological arguments rule out the development of a
chromosphere around black hole temperatures of order Lambda_QCD. In all cases,
the observational signatures of a cosmic or Galactic halo background of
primordial black holes or an individual black hole remain essentially those of
the standard Hawking model, with little change to the detection probability. We
also consider the possibility, as proposed by Belyanin et al. and D. Cline et
al., that plasma interactions between the emitted particles form a photosphere,
and we conclude that this scenario too is not supported.Comment: version published in Phys Rev D 78, 064043; 25 pages, 3 figures;
includes discussion on extending our analysis to TeV-scale,
higher-dimensional black hole
Multi-Parton Interactions at the LHC
We review the recent progress in the theoretical description and experimental
observation of multiple parton interactions. Subjects covered include
experimental measurements of minimum bias interactions and of the underlying
event, models of soft physics implemented in Monte Carlo generators,
developments in the theoretical description of multiple parton interactions and
phenomenological studies of double parton scattering. This article stems from
contributions presented at the Helmholtz Alliance workshop on "Multi-Parton
Interactions at the LHC", DESY Hamburg, 13-15 September 2010.Comment: 68 page
Forward Physics at the LHC (Elba 2010)
The papers review the main theoretical and experimental aspects of the
Forward Physics at the Large Hadron Collider
Determination of absolute neutrino masses from Z-bursts
Ultrahigh energy neutrinos (UHE\nu) scatter on relic neutrinos (R\nu)
producing Z bosons, which can decay hadronically producing protons (Z-burst).
We compare the predicted proton spectrum with the observed ultrahigh energy
cosmic ray (UHECR) spectrum and determine the mass of the heaviest R\nu via a
maximum likelihood analysis. Our prediction depends on the origin of the
power-like part of the UHECR spectrum: m_\nu=2.75^{+1.28}_{-0.97} eV for
Galactic halo and 0.26^{+0.20}_{-0.14} eV for extragalactic (EG) origin. The
necessary UHE\nu flux should be detected in the near future.Comment: slight rewording, revised neutrino fluxes, conclusions unchanged,
version to appear in Phys. Rev. Let
Calculation of parity and time invariance violation in the radium atom
Parity (P) and time (T) invariance violating effects in the Ra atom are
strongly enhanced due to close states of opposite parity, the large nuclear
charge Z and the collective nature of P,T-odd nuclear moments. We have
performed calculations of the atomic electric dipole moments (EDM) produced by
the electron EDM and the nuclear magnetic quadrupole and Schiff moments. We
have also calculated the effects of parity non-conservation produced by the
nuclear anapole moment and the weak charge. Our results show that as a rule the
values of these effects are much larger than those considered so far in other
atoms (enhancement is up to 10^5 times).Comment: 18 pages; LaTeX; Submitted to Phys. Rev.
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