activity
19982019
most citedSearching for long-lived particles beyond the Standard Model at the Large Hadron Collider

264 citations · 1.1k across the 19 of their papers we have counts for

collaborators

21 papers

hep-ex2019★ 264 cited

Searching for long-lived particles beyond the Standard Model at the Large Hadron Collider

Juliette Alimena, James Beacham, Martino Borsato +198

Particles beyond the Standard Model (SM) can generically have lifetimes that are long compared to SM particles at the weak scale. When produced at experiments such as the Large Had…

cond-mat.mes-hall2017★ 29 cited

Spin transport in two-layer-CVD-hBN/graphene/hBN heterostructures

Mallikarjuna Gurram, Siddhartha Omar, Simon Zihlmann +5

We study room temperature spin transport in graphene devices encapsulated between a layer-by-layer-stacked two-layer-thick chemical vapour deposition (CVD) grown hexagonal boron ni…

quant-ph2017★ 14 cited

Measurements of a Quantum Dot with an Impedance-Matching On-Chip LC Resonator at GHz Frequencies

M. -C. Harabula, T. Hasler, G. Fülöp +3

We report the realization of a bonded-bridge on-chip superconducting coil and its use in impedance-matching a highly ohmic quantum dot (QD) to a measurement setup. The…

astro-ph.SR2017★ 32 cited

Observing the metal-poor solar neighbourhood: a comparison of galactic chemical evolution predictions

T. Mishenina, M. Pignatari, B. Cot'e +14

Atmospheric parameters and chemical compositions for ten stars with metallicities in the region of -2.2< [Fe/H] <-0.6 were precisely determined using high resolution, high signal t…

astro-ph.SR2012

Nova Framework: A New Tool For Modeling of Nova Outbursts and Nucleosynthesis

Pavel A. Denissenkov, Falk Herwig, Marco Pignatari +1

Classical novae are the results of surface thermonuclear explosions of H-rich material accreted by white dwarfs (WDs) from their low-mass main-sequence or red-giant binary companio…

astro-ph2008

NuGrid: s process in massive stars

Raphael Hirschi, Urs Frischknecht, F. -K. Thielemann +10

The s-process production in massive stars at very low metallicities is expected to be negligible due to the low abundance of the neutron source 22Ne, to primary neutron poisons and…