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Daniele Ninci

Publications and source records attributed to Daniele Ninci.

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TD-Link: A Daisy-Chain Optical Architecture for Integrated Data Readout and Deterministic Timing Distribution in Large-Scale Detector Systems

TD-Link is a custom optical communication architecture that combines high-throughput data readout and sub-nanosecond timing synchronization over a single optical fiber for large-scale detector systems. The protocol adopts a multidrop daisy-chain ring topology connecting a Data Concentrator to up to sixteen FERS front-end boards per link, with up to eight independent links per concentrator. Operating at 3.125~Gb/s, TD-Link carries data, synchronization, and control traffic within the same serial stream through a token-based streaming protocol that minimizes per-hop latency and supports on-the-fly payload fragmentation. Transmitter lane alignment on the concentrator is achieved by exploiting the half-full condition of the multi-gigabit transceiver elastic buffer as a one-bit phase detector: a firmware finite-state machine iteratively adjusts the transmit phase interpolator until the FIFO write-to-read pointer difference reaches half-depth, locking each lane to a deterministic phase condition. A Digital Dual Mixer Time Difference (DDMTD) circuit is employed for inter-concentrator synchronization, measuring and compensating the phase offset between the recovered transceiver clock and the FPGA fabric reference clock. On the FERS boards, the recovered clock is cleaned by an external zero-delay PLL and retransmitted downstream, preserving phase coherence along the daisy chain. Experimental validation with CERN PicoTDC-equipped FERS boards demonstrates a board-to-board synchronization sigma of 7~ps for boards sharing a coaxial reference clock and below 28~ps for boards on independent concentrators. The results are stable across power cycles, confirming the robustness of the alignment strategy.

physics.ins-det

Search for Dark Matter decay signals in the Galactic Halo with the MAGIC telescopes

MAGIC is a system of two Cherenkov telescopes located in the Canary island of La Palma. A key part of MAGIC Fundamental Physics program is the search for indirect signals of Dark Matter (DM) from different sources. In the Milky Way, DM forms an almost spherically symmetric halo, with a density peaked towards the center of the Galaxy and decreasing toward the outer region. We search for DM decay signals from the Galactic Halo, with a special methodology developed for this work. Our strategy is to compare pairs of observations performed at different angular distances from the Galactic Center, selected in such a way that all the diffuse components cancel out, except for those coming from the DM. In order to keep the systematic uncertainty of this novel background estimation method down to a minimum, the observation pairs have been acquired during the same nights and follow exactly the same azimuth and zenith paths. We collected 20 hours of data during 2018. Using half of them to determine the systematic uncertainty in the background estimation of our analysis, we obtain a value of 4.8\% with no dependence on energy. Accounting for this systematic uncertainty in the likelihood analysis based on the 10 remaining hours of data collected so far, we present the limit to TeV DM particle with a lifetime of $10^{26}$ s in the $\mathrm{b\bar{b}}$ decay channel.

astro-ph.HE