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| name = Chuck Gallo
| name = Chuck Gallo
| alt = Chuck Gallo
| alt = Chuck Gallo
| birth_date = {{birth date|1935|00|00|mf=y}}
| birth_date = 1935
| residence = Lake Elmo, MN, United States
| residence = Lake Elmo, MN, United States
| known_for = [[Asronomy]], [[Big Bang]]
| nationality = American
| fields = [[Physics]], [[Astronomy]]
| workplaces = Superconix, Inc.
| known_for = Galactic rotation curves, alternatives to [[Dark matter]]
}}
}}


Superconix, Inc.
'''Charles F. "Chuck" Gallo''' (born 1935) is an American physicist based in Lake Elmo, Minnesota. He is president and founder of Superconix, Inc., a research and development company, and is known for his work modeling the rotation of spiral galaxies using classical Newtonian gravity without invoking [[Dark matter]].
 
==Biography==
Gallo is a physicist whose career has spanned applied research in superconductors, materials science and astrophysics. He founded and directs Superconix, Inc., a research and development laboratory in Lake Elmo, Minnesota. Much of his published astronomical work has been carried out in collaboration with James Q. Feng of Superconix, Inc.
 
==Work==
Gallo's research addresses the rotation of spiral galaxies. Working with James Q. Feng, he developed thin-disk gravitational models that seek to reproduce the observed flat rotation curves of spiral galaxies by balancing Newtonian gravitational and centrifugal forces within a rotating disk, rather than assuming a spherically symmetric halo of unseen matter. Their models numerically solve for the mass distribution required to match a measured rotation curve, and conclude that the flat rotation profiles correspond to mass density that decreases approximately exponentially from the galactic center, with relatively more ordinary baryonic mass in the cooler outer regions of a galaxy.
 
Gallo and Feng argue that describing a rotating disk galaxy with a spherically symmetric mass model can lead to erroneous conclusions, and they present their disk-based analysis as an alternative to the hypothesis of large amounts of non-baryonic dark matter. Related work by Gallo has also proposed a spiral galaxy model incorporating an axial plasma or gas vortex.
 
Their studies appear in journals including ''Research in Astronomy and Astrophysics'' and ''Galaxies'', in addition to preprints and conference presentations.
 
'''Selected publications:'''
 
* J. Q. Feng and C. F. Gallo, "Galactic Rotation Described with Thin-Disk Gravitational Model," [https://arxiv.org/abs/0803.0556 arXiv:0803.0556] (2008).
* J. Q. Feng and C. F. Gallo, "Modeling the Newtonian dynamics for rotation curve analysis of thin-disk galaxies," ''Research in Astronomy and Astrophysics'', 2011.
* C. F. Gallo and J. Q. Feng, "Mass Distribution in Rotating Thin-Disk Galaxies According to Newtonian Dynamics," ''Galaxies'', 2014.
* J. Q. Feng and C. F. Gallo, "Rotating Disk Galaxies without Dark Matter Based on Scientific Reasoning," ''Galaxies'', 2020.


'''Abstracts:'''
'''Abstracts:'''
Line 14: Line 34:
* Gallo and Feng, E12.00005, [http://meetings.aps.org/Meeting/APR07/Event/64814 Rotation of Spiral Galaxies Described with Various Sphere/Disc Gravitational Models]
* Gallo and Feng, E12.00005, [http://meetings.aps.org/Meeting/APR07/Event/64814 Rotation of Spiral Galaxies Described with Various Sphere/Disc Gravitational Models]
* Gallo, S1.00009, [http://meetings.aps.org/Meeting/APR07/Event/65523 Spiral Galaxy Model with Axial Plasma/Gas Vortex: A Possible Suggestion]
* Gallo, S1.00009, [http://meetings.aps.org/Meeting/APR07/Event/65523 Spiral Galaxy Model with Axial Plasma/Gas Vortex: A Possible Suggestion]
==External links==
* [https://arxiv.org/a/gallo_c_1 Charles F. Gallo on arXiv]


[[Category:Scientist|Gallo Charles]]
[[Category:Scientist|Gallo Charles]]
[[Category:Astronomy]]

Latest revision as of 09:39, 20 July 2026

Chuck Gallo
Born1935
ResidenceLake Elmo, MN, United States
NationalityAmerican
Known forGalactic rotation curves, alternatives to Dark matter
Scientific career
FieldsPhysics, Astronomy
InstitutionsSuperconix, Inc.

Charles F. "Chuck" Gallo (born 1935) is an American physicist based in Lake Elmo, Minnesota. He is president and founder of Superconix, Inc., a research and development company, and is known for his work modeling the rotation of spiral galaxies using classical Newtonian gravity without invoking Dark matter.

Biography

Gallo is a physicist whose career has spanned applied research in superconductors, materials science and astrophysics. He founded and directs Superconix, Inc., a research and development laboratory in Lake Elmo, Minnesota. Much of his published astronomical work has been carried out in collaboration with James Q. Feng of Superconix, Inc.

Work

Gallo's research addresses the rotation of spiral galaxies. Working with James Q. Feng, he developed thin-disk gravitational models that seek to reproduce the observed flat rotation curves of spiral galaxies by balancing Newtonian gravitational and centrifugal forces within a rotating disk, rather than assuming a spherically symmetric halo of unseen matter. Their models numerically solve for the mass distribution required to match a measured rotation curve, and conclude that the flat rotation profiles correspond to mass density that decreases approximately exponentially from the galactic center, with relatively more ordinary baryonic mass in the cooler outer regions of a galaxy.

Gallo and Feng argue that describing a rotating disk galaxy with a spherically symmetric mass model can lead to erroneous conclusions, and they present their disk-based analysis as an alternative to the hypothesis of large amounts of non-baryonic dark matter. Related work by Gallo has also proposed a spiral galaxy model incorporating an axial plasma or gas vortex.

Their studies appear in journals including Research in Astronomy and Astrophysics and Galaxies, in addition to preprints and conference presentations.

Selected publications:

  • J. Q. Feng and C. F. Gallo, "Galactic Rotation Described with Thin-Disk Gravitational Model," arXiv:0803.0556 (2008).
  • J. Q. Feng and C. F. Gallo, "Modeling the Newtonian dynamics for rotation curve analysis of thin-disk galaxies," Research in Astronomy and Astrophysics, 2011.
  • C. F. Gallo and J. Q. Feng, "Mass Distribution in Rotating Thin-Disk Galaxies According to Newtonian Dynamics," Galaxies, 2014.
  • J. Q. Feng and C. F. Gallo, "Rotating Disk Galaxies without Dark Matter Based on Scientific Reasoning," Galaxies, 2020.

Abstracts:

External links