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researcher

C. Lunardini

70 papers hereh-index 343.5k citations107 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • sole author7
  • first author18
  • middle author22
  • last author20

Across the 67 of 70 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE29
  • hep-ph22
  • astro-ph.CO6
  • astro-ph5
  • astro-ph.SR4
  • nucl-th2
same name
  • C. Lunardini — 1 paper, h 0

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20002026
most citedPhysics at a future Neutrino Factory and super-beam facility

254 citations · 3.5k across the 69 of their papers we have counts for

collaborators
Showing 2000Show all

4 papers · 1 filter

hep-ph2000★ 66 cited

Neutrinos from SN1987A, Earth matter effects and the LMA solution of the solar neutrino problem

C. Lunardini, A. Yu. Smirnov

We study properties of the oscillation effects in the matter of the Earth on antineutrino fluxes from supernovae. We show that these effects can provide explanation of the differen…

hep-ph2000★ 141 cited

Large-angle Bhabha scattering and luminosity at flavour factories

C. M. Carloni Calame, C. Lunardini, G. Montagna +2

The luminosity determination of electron-positron colliders operating in the region of low-lying hadronic resonances (E_cm ~ 1-10 GeV), such as BEPC/BES, DAPHNE, KEKB, PEP-II and V…

hep-ph2000★ 45 cited

The minimum width condition for neutrino conversion in matter

C. Lunardini, A. Yu. Smirnov

We find that for small vacuum mixing angle θ and low energies (s≪MZ2​) the width of matter, d1/2​, needed to have conversion probability P≥1/2 should be larger th…

hep-ph2000★ 1 cited

Large-angle Bhabha scattering and luminosity at Daphne

C. M. Carloni Calame, C. Lunardini, G. Montagna +2

The accurate knowledge of luminosity at e^+ e^- flavour factories requires the precision calculation of the Bhabha cross section at large scattering angles. In order to achieve a t…

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