Satoshi Iso

4.3k total citations
87 papers, 2.9k citations indexed

About

Satoshi Iso is a scholar working on Nuclear and High Energy Physics, Astronomy and Astrophysics and Statistical and Nonlinear Physics. According to data from OpenAlex, Satoshi Iso has authored 87 papers receiving a total of 2.9k indexed citations (citations by other indexed papers that have themselves been cited), including 67 papers in Nuclear and High Energy Physics, 44 papers in Astronomy and Astrophysics and 33 papers in Statistical and Nonlinear Physics. Recurrent topics in Satoshi Iso's work include Black Holes and Theoretical Physics (56 papers), Cosmology and Gravitation Theories (44 papers) and Noncommutative and Quantum Gravity Theories (25 papers). Satoshi Iso is often cited by papers focused on Black Holes and Theoretical Physics (56 papers), Cosmology and Gravitation Theories (44 papers) and Noncommutative and Quantum Gravity Theories (25 papers). Satoshi Iso collaborates with scholars based in Japan, United States and South Korea. Satoshi Iso's co-authors include Hiroshi Umetsu, Yuta Orikasa, Hajime Aoki, Nobuchika Okada, Frank Wilczek, H. Kawai, Yoshihisa Kitazawa, Takeshi Morita, Nobuyuki Ishibashi and Tsukasa Tada and has published in prestigious journals such as Physical Review Letters, Physical review. B, Condensed matter and Physical Review B.

In The Last Decade

Satoshi Iso

80 papers receiving 2.8k citations

Peers — A (Enhanced Table)

Peers by citation overlap · career bar shows stage (early→late) cites · hero ref

Name h Career Trend Papers Cites
Satoshi Iso Japan 29 2.3k 1.6k 1.2k 944 205 87 2.9k
Djordje Minić United States 28 2.6k 1.1× 2.1k 1.3× 1.9k 1.7× 812 0.9× 158 0.8× 105 3.3k
V. P. Nair United States 35 3.3k 1.4× 1.2k 0.7× 1.5k 1.3× 1.1k 1.2× 370 1.8× 136 4.0k
P. A. Horváthy France 27 1.7k 0.7× 1.1k 0.7× 1.3k 1.1× 1.0k 1.1× 191 0.9× 129 2.6k
Johanna Erdmenger Germany 28 3.1k 1.3× 2.2k 1.4× 907 0.8× 638 0.7× 117 0.6× 112 3.5k
Y. Jack Ng United States 27 1.8k 0.7× 1.2k 0.8× 791 0.7× 694 0.7× 102 0.5× 105 2.5k
Dimitra Karabali United States 23 1.7k 0.7× 387 0.2× 731 0.6× 956 1.0× 286 1.4× 56 2.4k
Kristan Jensen United States 25 2.0k 0.9× 1.4k 0.9× 852 0.7× 749 0.8× 109 0.5× 53 2.5k
Constantin P. Bachas France 26 2.8k 1.2× 1.5k 0.9× 1.0k 0.9× 256 0.3× 377 1.8× 65 3.1k
G. W. Semenoff Canada 19 1.6k 0.7× 541 0.3× 639 0.6× 1.1k 1.1× 135 0.7× 53 2.4k
Zohar Komargodski United States 30 2.8k 1.2× 1.4k 0.9× 898 0.8× 510 0.5× 357 1.7× 51 3.2k

Countries citing papers authored by Satoshi Iso

Since Specialization
Citations

This map shows the geographic impact of Satoshi Iso'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 Satoshi Iso with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Satoshi Iso more than expected).

Fields of papers citing papers by Satoshi Iso

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by Satoshi Iso. 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 Satoshi Iso. The network helps show where Satoshi Iso may publish in the future.

Co-authorship network of co-authors of Satoshi Iso

This figure shows the co-authorship network connecting the top 25 collaborators of Satoshi Iso. A scholar is included among the top collaborators of Satoshi Iso 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 Satoshi Iso. Satoshi Iso is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

20 of 20 papers shown
1.
Hidaka, Yoshimasa, et al.. (2023). Entanglement generation and decoherence in a two-qubit system mediated by relativistic quantum field. Physical review. D. 107(8). 5 indexed citations
2.
Iso, Satoshi, et al.. (2021). Entanglement entropy in scalar field theory and ZM gauge theory on Feynman diagrams. Physical review. D. 103(10). 8 indexed citations
3.
Iso, Satoshi, et al.. (2021). Wilsonian Effective Action and Entanglement Entropy. Symmetry. 13(7). 1221–1221. 8 indexed citations
4.
Iso, Satoshi, et al.. (2017). QCD-Electroweak First-Order Phase Transition in a Supercooled Universe. Physical Review Letters. 119(14). 141301–141301. 93 indexed citations
5.
Asaka, T., Satoshi Iso, H. Kawai, et al.. (2016). Reinterpretation of the Starobinsky model. Progress of Theoretical and Experimental Physics. 2016(12). 123E01–123E01. 18 indexed citations
6.
Hashimoto, Michio, Satoshi Iso, & Yuta Orikasa. (2014). Radiative symmetry breaking from flat potential in variousU(1)models. Physical review. D. Particles, fields, gravitation, and cosmology. 89(5). 35 indexed citations
7.
Aoki, Hajime & Satoshi Iso. (2012). Revisiting the naturalness problem: Who is afraid of quadratic divergences?. Physical review. D. Particles, fields, gravitation, and cosmology. 86(1). 51 indexed citations
8.
Iso, Satoshi, Nobuchika Okada, & Yuta Orikasa. (2011). Resonant leptogenesis in the minimalBLextended standard model at TeV. Physical review. D. Particles, fields, gravitation, and cosmology. 83(9). 44 indexed citations
9.
Iso, Satoshi, Nobuchika Okada, & Yuta Orikasa. (2009). MinimalBLmodel naturally realized at the TeV scale. Physical review. D. Particles, fields, gravitation, and cosmology. 80(11). 159 indexed citations
10.
Iso, Satoshi, et al.. (2009). Generalized conformal symmetry and recovery of SO(8) in multiple M2 and D2 branes. Nuclear Physics B. 816(1-2). 256–277. 9 indexed citations
11.
Iso, Satoshi, Hiroshi Umetsu, & Frank Wilczek. (2006). Hawking Radiation from Charged Black Holes via Gauge and Gravitational Anomalies. Physical Review Letters. 96(15). 151302–151302. 178 indexed citations
12.
Iso, Satoshi & Hiroshi Umetsu. (2004). Gauge theory on a noncommutative supersphere from a supermatrix model. Physical review. D. Particles, fields, gravitation, and cosmology. 69(10). 22 indexed citations
13.
Aoki, Hajime, Nobuyuki Ishibashi, Satoshi Iso, et al.. (2000). Non-commutative Yang–Mills in IIB matrix model. Nuclear Physics B. 565(1-2). 176–192. 151 indexed citations
14.
Ishibashi, Nobuyuki, Satoshi Iso, H. Kawai, & Yoshihisa Kitazawa. (2000). String scale in noncommutative Yang–Mills. Nuclear Physics B. 583(1-2). 159–181. 24 indexed citations
15.
Ishibashi, Nobuyuki, Satoshi Iso, H. Kawai, & Yoshihisa Kitazawa. (2000). Wilson loops in non-commutative Yang–Mills. Nuclear Physics B. 573(1-2). 573–593. 124 indexed citations
16.
Aoki, Hajime, Satoshi Iso, H. Kawai, et al.. (1999). IIB Matrix Model. Progress of Theoretical Physics Supplement. 134. 47–83. 72 indexed citations
17.
Iso, Satoshi. (1995). Anyon basis of c = 1 conformal field theory. Nuclear Physics B. 443(3). 581–595. 24 indexed citations
18.
Aoki, Hajime, et al.. (1994). The Effect of Dynamical Gauge Field on the Chiral Fermion on a Boundary. 10 indexed citations
19.
Iso, Satoshi. (1992). Phase-Space and Symplectic Structure of the Fractional Quantum Hall Effect. Progress of Theoretical Physics. 87(1). 111–125.
20.
Iso, Satoshi, et al.. (1990). The spin factor in knots and a relativistic treatment of the Bose-Fermi trasmutation in second-quantized theories. Nuclear Physics B. 346(2-3). 293–312. 20 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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