دورية أكاديمية

A machian model as potential alternative to dark matter halo thesis in galactic rotational velocity prediction.

التفاصيل البيبلوغرافية
العنوان: A machian model as potential alternative to dark matter halo thesis in galactic rotational velocity prediction.
المؤلفون: Walrand, Stephan, Arbañil Vela, José Domingo, Benedetto, Elmo
المصدر: Frontiers in Astronomy & Space Sciences; 2024, p01-07, 7p
مصطلحات موضوعية: DARK matter, INERTIAL mass, CENTRIFUGAL force, EINSTEIN field equations, VELOCITY, GRAVITATIONAL fields, GALACTIC halos
مستخلص: A novel axially symmetric metric is proposed to solve the Einstein field equations. This provides an analytical solution within the matter in the equatorial plane for any galaxy density profile. The solution predicts the observed increase in rotational velocity up to the edge of the galaxy's bulge. However, beyond the bulge, the rotational velocity remains constant, which contradicts the observed peak curves. The existence of the Universe is then considered by approximating the gravitational fields within the galaxy as the sum of those generated by the galaxy and the Universe. The resulting solution explicitly includes a Universe frame-dragging term, aligning with the sixth version of Mach's principle proposed by Bondi and Samuel: "inertial mass is affected by the global distribution of matter". Neglecting the presence of the Universe, stars only have a relative rotation to the bulge, and their rotational velocities monotonically increase with the radial distance r to balance the increasing mass contained in distances < r. At larger distances, the bulge's attraction and its frame-dragging effect decrease, resulting in a constant rotational velocity. When the Universe is considered, stars also have a relative rotation to the non-rotating Universe and experience an additional centrifugal force at any distance from the bulge. This component induces a decrease in rotational velocity as the gravitational influence of the bulge diminishes with r. This model predicts the observed rotational velocity curves for the galaxies M31, M101, and M81 without requiring any dark matter halo or adjustable parameters. This success substantiates Mach's idea as an alternative to the dark matter halo theory. [ABSTRACT FROM AUTHOR]
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قاعدة البيانات: Complementary Index
الوصف
تدمد:2296987X
DOI:10.3389/fspas.2024.1429235