The gravitational field of the electron
Physics Letters A, ISSN: 0375-9601, Vol: 32, Issue: 6, Page: 402-403
1970
- 7Citations
- 1Usage
- 1Captures
- 1Mentions
Metric Options: CountsSelecting the 1-year or 3-year option will change the metrics count to percentiles, illustrating how an article or review compares to other articles or reviews within the selected time period in the same journal. Selecting the 1-year option compares the metrics against other articles/reviews that were also published in the same calendar year. Selecting the 3-year option compares the metrics against other articles/reviews that were also published in the same calendar year plus the two years prior.
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Example: if you select the 1-year option for an article published in 2019 and a metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019. If you select the 3-year option for the same article published in 2019 and the metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019, 2018 and 2017.
Citation Benchmarking is provided by Scopus and SciVal and is different from the metrics context provided by PlumX Metrics.
Metrics Details
- Citations7
- Citation Indexes7
- CrossRef7
- Usage1
- Abstract Views1
- Captures1
- Readers1
- Mentions1
- References1
- Wikipedia1
Article Description
We show that spin contributions to the gravitational field of an electron dominate for distances between the classical radius and the Compton wavelength of the electron. At such distances the gravitational force between two electrons may be repulsive, depending on the spin orientations.
Bibliographic Details
http://www.sciencedirect.com/science/article/pii/0375960170900228; http://dx.doi.org/10.1016/0375-9601(70)90022-8; http://www.scopus.com/inward/record.url?partnerID=HzOxMe3b&scp=49849109278&origin=inward; https://linkinghub.elsevier.com/retrieve/pii/0375960170900228; https://api.elsevier.com/content/article/PII:0375960170900228?httpAccept=text/xml; https://api.elsevier.com/content/article/PII:0375960170900228?httpAccept=text/plain; https://repository.lsu.edu/physics_astronomy_pubs/4096; https://repository.lsu.edu/cgi/viewcontent.cgi?article=5176&context=physics_astronomy_pubs; http://dx.doi.org/10.1016/0375-9601%2870%2990022-8; https://dx.doi.org/10.1016/0375-9601%2870%2990022-8
Elsevier BV
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