activity
20092021
most citedCopernicanism and the Typicality in Time

19 citations · 155 across the 15 of their papers we have counts for

collaborators

16 papers

hep-ex2021★ 14 cited

meson production in inelastic interactions at 158 GeV/c beam momentum measured by NA61/SHINE at the CERN SPS

A. Acharya, H. Adhikary, K. K. Allison +139

The production of mesons in inelastic collisions at beam momentum 158 GeV/c ( GeV) was measured with the NA61/SHINE spectrometer at t…

nucl-ex2021

Measurements of and production in proton-proton interactions at = 17.3 GeV in the NA61/SHINE experiment

A. Acharya, H. Adhikary, K. K. Allison +140

Double-differential yields of and resonances produced in \pp interactions were measured at a laboratory beam momentum of…

astro-ph.IM2021★ 19 cited

Longevity is the key factor in the search for technosignatures

Amedeo Balbi, Milan M. Ćirković

It is well-known that the chances of success of SETI depend on the longevity of technological civilizations or, more broadly, on the duration of the signs of their existence, or te…

hep-ex2021

Spectra and mean multiplicities of in Ar+Sc collisions at 13, 19, 30, 40, 75 and 150 GeV/ beam momenta measured by the NA61/SHINE spectrometer at the CERN SPS

SHINE collaboration, A. Acharya, H. Adhikary +139

The physics goal of the strong interaction program of the NA61/SHINE experiment at the CERN Super Proton Synchrotron (SPS) is to study the phase diagram of hadronic matter by a sca…

nucl-ex2020★ 4 cited

Measurements of multiplicity fluctuations of identified hadrons in inelastic proton-proton interactions at the CERN Super Proton Synchrotron

SHINE Collaboration, A. Acharya, H. Adhikary +139

Measurements of multiplicity fluctuations of identified hadrons produced in inelastic p+p interactions at 31, 40, 80, and 158~\GeVc beam momentum are presented. Three different mea…

physics.pop-ph2020★ 1 cited

Habitability of M dwarfs is a problem for the traditional SETI

Milan M. Ćirković, Branislav Vukotić

We consider some implications of the much-discussed circumstellar habitable zones around M-dwarf stars for the conventionally understood radio SETI. We argue that the flaring natur…