[Alumnes] HOY 13:00hs - Seminario FCAG - Lic. Tobías Canavesi - (FCAG-IFLP-CONICET)
Secretaría de Ciencia y Técnica
secyt en fcaglp.unlp.edu.ar
Mie Sep 25 08:20:06 -03 2019
Estimados,
Les recordamos que en el día de hoy, a las 13:00 hs. en el Salón
Meridiano, tendremos un Seminario a cargo del Lic. Tobías Canavesi
(FCAG-IFLP-CONICET) *, el cual **se titula "Fractal Gravitation ." El
**resumen del mismo lo pueden leer al final de este mensaje.*
****
**Les recordamos, además, que los objetivos de estos seminarios son el
de generar un espacio ameno y activo de intercambio de ideas, para
exponer nuestros trabajos y temas de investigación, o bien el de
aquellos que circunstancialmente nos visitan en nuestra casa de altos
estudios. Teniendo en cuenta que nuestra institución nuclea una gran
diversidad de temas de investigación, y distintos estamentos académicos,
este espacio resulta de vital importancia para conocernos, acercarnos y
hasta generar posibles colaboraciones. **
*******
**Quedan todos cordialmente invitados y los esperamos 15 minuto**s antes
con café y galletitas.
**Atentamente,
**
**Secyt-FCAG**
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Título:Fractal Gravitation
Seminario: Lic. Tobias Canavesi (FCAG-IFLP-CONICET)
Resumen: A new effective theory of modified gravity is presented and
axiomatized. In this theory we start from a generalized Poisson equation
and proposed a modification physical dimension by a fractal dimension,
since we find using the data from gaia second release that the stars in
the Milky Way are distributed in a fractal way, checking what was
already thought Elmegreen(2000). We tested the model to calculate
circular velocities for several galaxies including the Milky Way. For
doing this, two numerical models were used, the first considering
uniform density and the second more realistic with a bulge and a disc
proposed by Scelza, G. & Stabile, A.(2015), but without density of dark
matter, and adapted for our fractal potential. We tested the simplest
model in 14 low surface brightness galaxies, taken from the work de
Blok, W. J. G., & Bosma, A. (2002). We use the bulge and disk model for
the spiral galaxies NGC 300 (SA (s)d), NGC 247 (SAB (s)d), then we make
a comparison with the adjustment given by Newton's Theory of Universal
Gravitation.
Finally, we study the case of the Milky Way in a detailed manner, taking
into account that for it we have more data than for the galaxies
mentioned above. First we calculated the fractal dimension using the
box-counting dimension for a around the barycenter of the solar system
using the data from the second release of gaia and the distances
calculated by Bailer-Jones, C. A.(2018), for 999997 stars. To conclude,
we study its validity by contrasting the data for the circular velocity
of the Milky Way obtained from the works of Huang, Y.(2016) and Pato,
M., & Iocco, F. (2017).
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