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researcher

A. Drago

95 papers hereh-index 366.5k citations391 works total

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

author position
  • sole author5
  • first author31
  • middle author44
  • last author9

Across the 89 of 95 papers where every author was matched, so the position is known.

fields
  • physics.acc-ph22
  • hep-ph18
  • astro-ph.HE16
  • nucl-th15
  • astro-ph12
  • astro-ph.SR5
same name
  • A. Drago — 16 papers, h 6
  • A. Drago — 7 papers
  • A. Drago — 6 papers, h 8
  • A. Drago — 3 papers, h 4
  • A. Drago — 3 papers, h 1
  • A. Drago — 3 papers, h 3

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
19952023
most citedTransverse Polarisation of Quarks in Hadrons

460 citations · 2.5k across the 90 of their papers we have counts for

collaborators
Showing 2001Show all

4 papers · 1 filter

physics.acc-ph2001★ 6 cited

Fast Electronics for the Dafne Transverse Feedback Systems

A. Drago, A. Argan, M. Serio

Transverse feedback systems for controlling the vertical coupled-bunch instabilities in the positron and electron main rings are installed at DAFNE. They started to be operative re…

hep-ph2001★ 13 cited

Stability of strange quark matter: MIT bag versus Color Dielectric Model

W. M. Alberico, A. Drago, C. Ratti

We discuss the properties of strange matter, in particular the minimum of the energy per baryon number as a function of the strangeness fraction. We utilize both the MIT bag model…

hep-ph2001★ 460 cited

Transverse Polarisation of Quarks in Hadrons

Vincenzo Barone, Alessandro Drago, Philip G. Ratcliffe

We review the present state of knowledge regarding the transverse polarisation (or transversity) distributions of quarks. After some generalities on transverse polarisation, we for…

hep-ph2001★ 43 cited

From Quark Stars to Hybrid Stars

Alessandro Drago, Andrea Lavagno

We show the possible existence of compact stars having a surface composed of a mixed phase of quarks and hadrons. This scenario can be realized both for self-bound stars, satisfyin…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.