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Analysis of institutional authors

Chamizo FCorresponding Author

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Current induction and macroscopic forces for superconducting strings

Publicated to:PHYSICAL REVIEW D. 107 (7): e075015- - 2023-04-01 107(7), DOI: 10.1103/PhysRevD.107.075015

Authors: Chamizo, F.; Santillán, O.P.

Affiliations

UBA CONICET, Inst Matemat Luis Santalo IMAS, Buenos Aires, Argentina - Author
Univ Autonoma Madrid, Dept Matemat, Madrid 28049, Spain - Author
Univ Autonoma Madrid, ICMAT, Madrid 28049, Spain - Author
Universidad Autónoma de Madrid - Author
Universidad de Buenos Aires - Author
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Abstract

Superconducting strings are topological defects appearing in cosmological early stage models, in tentative explanations of the high energy cosmic rays, galaxy formation and even in condensed matter to deal with some kind of superconductors. The main topic studied in this paper is the inverse photoelectric effect for superconducting lines namely, it is estimated the cross section corresponding to the adsorption of a fermion with the consequent emission of a photon. This issue is of importance, as some of these fermions can become a zero mode inside the core of the object, thus traveling at the speed of light and generating a possibly large current, whose cosmological implications has been discussed in a variety of works. A discussion is introduced comparing it to the Aharonov-Bohm cross section and relating them to the associated (Magnus) forces. It is also obtained a quite explicit description of the bound states and a version of Weyl's law for the energies.

Keywords

collapsecosmic stringsdynamicsfermi superfluidsinertial massmagnus forcequantized vortextransverse forcezero modesMutual friction

Quality index

Bibliometric impact. Analysis of the contribution and dissemination channel

The work has been published in the journal PHYSICAL REVIEW D due to its progression and the good impact it has achieved in recent years, according to the agency WoS (JCR), it has become a reference in its field. In the year of publication of the work, 2023, it was in position 17/84, thus managing to position itself as a Q1 (Primer Cuartil), in the category Astronomy & Astrophysics.

Impact and social visibility

From the perspective of influence or social adoption, and based on metrics associated with mentions and interactions provided by agencies specializing in calculating the so-called "Alternative or Social Metrics," we can highlight as of 2025-06-27:

With a more dissemination-oriented intent and targeting more general audiences, we can observe other more global scores such as:

  • The Total Score from Altmetric: 0.25.
  • The number of mentions on the social network X (formerly Twitter): 1 (Altmetric).

It is essential to present evidence supporting full alignment with institutional principles and guidelines on Open Science and the Conservation and Dissemination of Intellectual Heritage. A clear example of this is:

  • The work has been submitted to a journal whose editorial policy allows open Open Access publication.
  • Assignment of a Handle/URN as an identifier within the deposit in the Institutional Repository: https://repositorio.uam.es/handle/10486/707684

Leadership analysis of institutional authors

This work has been carried out with international collaboration, specifically with researchers from: Argentina.

There is a significant leadership presence as some of the institution’s authors appear as the first or last signer, detailed as follows: First Author (CHAMIZO LORENTE, FERNANDO) .

the author responsible for correspondence tasks has been CHAMIZO LORENTE, FERNANDO.