G. Cavallo

405 total citations
17 papers, 237 citations indexed

About

G. Cavallo is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Radiation. According to data from OpenAlex, G. Cavallo has authored 17 papers receiving a total of 237 indexed citations (citations by other indexed papers that have themselves been cited), including 13 papers in Astronomy and Astrophysics, 9 papers in Nuclear and High Energy Physics and 3 papers in Radiation. Recurrent topics in G. Cavallo's work include Astrophysics and Cosmic Phenomena (8 papers), Gamma-ray bursts and supernovae (5 papers) and Solar and Space Plasma Dynamics (3 papers). G. Cavallo is often cited by papers focused on Astrophysics and Cosmic Phenomena (8 papers), Gamma-ray bursts and supernovae (5 papers) and Solar and Space Plasma Dynamics (3 papers). G. Cavallo collaborates with scholars based in Italy, United States and Russia. G. Cavallo's co-authors include M. J. Rees, Robert J. Gould, A. Ventura, J. V. Jelley, Arcangelo Messina, G. G. C. Palumbo and Peter G. Craven and has published in prestigious journals such as Nature, The Astrophysical Journal and Monthly Notices of the Royal Astronomical Society.

In The Last Decade

G. Cavallo

16 papers receiving 229 citations

Peers

G. Cavallo
M. Kafatos United States
F. Seward United States
Ko Aizu Japan
W. B. McAdam Australia
C. Alcock United States
S. Tapia United States
T. J. Mazurek United States
L. Ensman United States
M. Kafatos United States
G. Cavallo
Citations per year, relative to G. Cavallo G. Cavallo (= 1×) peers M. Kafatos

Countries citing papers authored by G. Cavallo

Since Specialization
Citations

This map shows the geographic impact of G. Cavallo's research. It shows the number of citations coming from papers published by authors working in each country. You can also color the map by specialization and compare the number of citations received by G. Cavallo with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites G. Cavallo more than expected).

Fields of papers citing papers by G. Cavallo

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by G. Cavallo. Nodes represent research fields, and links connect fields that are likely to share authors. Colored nodes show fields that tend to cite the papers produced by G. Cavallo. The network helps show where G. Cavallo may publish in the future.

Co-authorship network of co-authors of G. Cavallo

This figure shows the co-authorship network connecting the top 25 collaborators of G. Cavallo. A scholar is included among the top collaborators of G. Cavallo based on the total number of citations received by their joint publications. Widths of edges represent the number of papers authors have co-authored together. Node borders signify the number of papers an author published with G. Cavallo. G. Cavallo is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

17 of 17 papers shown
1.
Cavallo, G., et al.. (1981). Spectrum of cosmic fireballs. Astrophysics and Space Science. 75(1). 117–123. 1 indexed citations
2.
Craven, Peter G., G. Cavallo, & G. G. C. Palumbo. (1978). A maximum likelihood estimate of the supernova rate in Sc galaxies.. 64. 87–90. 1 indexed citations
3.
Cavallo, G. & M. J. Rees. (1978). A qualitative study of cosmic fireballs and  -ray bursts. Monthly Notices of the Royal Astronomical Society. 183(3). 359–365. 170 indexed citations
4.
Cavallo, G.. (1978). On the sources of ultra-high energy cosmic rays.. 65. 415. 6 indexed citations
5.
Cavallo, G. & A. Ventura. (1975). Qualitative features of synchrotron radiation in an inhomogeneous magnetic field. Nature. 258(5533). 309–310. 1 indexed citations
6.
Cavallo, G. & J. V. Jelley. (1975). Why are no radio pulses associated with the bursts of celestial gamma-rays. The Astrophysical Journal. 201. L113–L113. 1 indexed citations
7.
Cavallo, G., et al.. (1975). The X and γ diffuse background. Rivista Del Nuovo Cimento. 5(2). 255–311. 7 indexed citations
8.
Cavallo, G. & Arcangelo Messina. (1974). On the initial energy of supernova remnants. Astrophysics and Space Science. 30(2). 409–416. 1 indexed citations
9.
Cavallo, G.. (1973). Nature of galactic x-ray sources. OSTI OAI (U.S. Department of Energy Office of Scientific and Technical Information). 41(4). 893–898.
10.
Cavallo, G.. (1973). Recent advances in short-time-constant astrophysics. Rivista Del Nuovo Cimento. 3(3). 205–232. 1 indexed citations
11.
Cavallo, G.. (1973). Interpretation of the Dirac Relationship between Fundamental Constants. Nature. 245(5424). 313–314. 6 indexed citations
12.
Cavallo, G. & A. Ventura. (1972). Restrictions on the short time constant astrophysics. Astrophysics and Space Science. 19(2). 431–439. 2 indexed citations
13.
Cavallo, G., et al.. (1972). Soft X-ray Background and Flare Stars. Nature Physical Science. 235(58). 110–110. 5 indexed citations
14.
Cavallo, G. & Robert J. Gould. (1971). A reply to Dr. Stecker’s comment. Lettere al nuovo cimento della societa italiana di fisica/Lettere al nuovo cimento. 2(23). 1199–1200. 1 indexed citations
15.
Cavallo, G.. (1971). Consideration of the Observed Isotropicγ-Ray Background. Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields. 3(2). 299–305. 1 indexed citations
16.
Cavallo, G. & Robert J. Gould. (1971). The neutral-pion decay and the gamma radiation from our galaxy. ˜Il œNuovo cimento della Società italiana di fisica. B/˜Il œNuovo cimento B. 2(1). 77–92. 31 indexed citations
17.
Cavallo, G.. (1971). Period–Luminosity Function for Pulsars. Nature Physical Science. 231(19). 35–36. 2 indexed citations

Rankless uses publication and citation data sourced from OpenAlex, an open and comprehensive bibliographic database. While OpenAlex provides broad and valuable coverage of the global research landscape, it—like all bibliographic datasets—has inherent limitations. These include incomplete records, variations in author disambiguation, differences in journal indexing, and delays in data updates. As a result, some metrics and network relationships displayed in Rankless may not fully capture the entirety of a scholar's output or impact.

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