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相关论文: Astrophysical Tests of Modified Gravity: Constrain…

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We calculate models of stellar evolution for very massive stars and include the effects of modified gravity to investigate the influence on the physical properties of blue supergiant stars and their use as extragalactic distance indicators.…

星系天体物理 · 物理学 2021-06-30 Eva Sextl , Rolf-Peter Kudritzki , Jochen Weller , Miguel A. Urbaneja , Achim Weiss

This paper is the third in a series on tests of gravity using observations of stars and nearby dwarf galaxies. We carry out four distinct tests using published data on the kinematics and morphology of dwarf galaxies, motivated by the…

宇宙学与河外天体物理 · 物理学 2015-06-15 Vinu Vikram , Anna Cabre , Bhuvnesh Jain , Jake VanderPlas

New theoretical evaluations of the Red Giant Branch Tip (TRGB) luminosity, by adopting the most updated physical inputs in computing canonical stellar models, are presented. Theoretical relations for the run of the TRGB bolometric and I…

天体物理学 · 物理学 2015-06-24 M. Salaris , S. Cassisi

The luminosity of the Tip of the Red Giant Branch (TRGB) provides an excellent measure of galaxy distances and is easily determined in the resolved images of nearby galaxies observed with Hubble Space Telescope. There is now a large amount…

In the nearby galaxy NGC 4258, the well-modeled orbital motion of H$_2$O masers about its supermassive black hole provides the means to measure a precise geometric distance. As a result, NGC 4258 is one of a few "geometric anchors"…

Astrophysical tests of modified modified gravity theories in the nearby universe have been emphasized recently by Hui, Nicolis and Stubbs (2009) and Jain and VanderPlas (2011). A key element of such tests is the screening mechanism whereby…

宇宙学与河外天体物理 · 物理学 2015-06-04 Anna Cabré , Vinu Vikram , Gong-Bo Zhao , Bhuvnesh Jain , Kazuya Koyama

The brightness of the tip of the red-giant branch (TRGB) allows one to constrain novel energy losses that would lead to a larger core mass at helium ignition and thus to a brighter TRGB than expected by standard stellar models. The required…

太阳与恒星天体物理 · 物理学 2021-03-25 Francesco Capozzi , Georg Raffelt

Modified theories of gravity provide us with a unique opportunity to generate innovative tests of gravity. In Chameleon f(R) gravity, the gravitational potential differs from the weak-field limit of general relativity (GR) in a mass…

宇宙学与河外天体物理 · 物理学 2016-04-26 Alejo Stark , Christopher J. Miller , Nicholas Kern , Daniel Gifford , Gong-Bo Zhao , Baojiu Li , Kazuya Koyama , Robert C. Nichol

Chameleon theories of gravity predict that the gaseous component of isolated dwarf galaxies rotates with a faster velocity than the stellar component. In this paper, we exploit this effect to obtain new constraints on the model parameters…

宇宙学与河外天体物理 · 物理学 2018-06-18 Vinu Vikram , Jeremy Sakstein , Charles Davis , Andrew Neil

Modified theories of gravity have received a renewed interest due to their ability to account for the cosmic acceleration. In order to satisfy the solar system tests of gravity, these theories need to include a screening mechanism that…

宇宙学与河外天体物理 · 物理学 2014-09-15 Jeremy Sakstein , Bhuvnesh Jain , Vinu Vikram

The extragalactic distance scale relies heavily on Cepheids. However, it has become clear from observations and pulsation models that the slope and zero point of their P-L relations differ from galaxy to galaxy. This makes the determination…

天体物理学 · 物理学 2009-11-13 G. A. Tammann , A. Sandage , B. Reindl

The tip of the red giant branch has been used to measure distances to 500 nearby galaxies with the Hubble Space Telescope (HST) which are available in the Color-Magnitude Diagrams and Tip of the Red Giant Branch (CMDs/TRGB) catalog on the…

宇宙学与河外天体物理 · 物理学 2022-06-15 Gagandeep S. Anand , R. Brent Tully , Luca Rizzi , Adam G. Riess , Wenlong Yuan

The Hubble Tension, a >5 sigma discrepancy between direct and indirect measurements of the Hubble constant (H0), has persisted for a decade and motivated intense scrutiny of the paths used to infer H0. Comparing independently-derived…

The local distance ladder measurement of the Hubble constant requires a connection between geometric distances at low redshift and Type Ia supernovae in the Hubble flow, which may be achieved through either the Cepheid period--luminosity…

宇宙学与河外天体物理 · 物理学 2020-07-15 Harry Desmond , Jeremy Sakstein

The TRGB-SBF Project team is developing an independent distance ladder using a geometrical calibration of the tip of the red giant branch (TRGB) method in elliptical galaxies that can in turn be used to set the surface brightness…

We present a revised TRGB calibration, accurate to 2.7% of distance. A modified TRGB magnitude corrected for the color dependence of the TRGB, the QT magnitude, is introduced for better measurement of the TRGB. We determine the…

星系天体物理 · 物理学 2017-01-25 In Sung Jang , Myung Gyoon Lee

The local determination of the Hubble Constant sits at a crossroad. Current estimates of the local expansion rate of the Universe differ by about 1.7-sigma, derived from the Cepheid and TRGB based calibrations, applied to type Ia…

宇宙学与河外天体物理 · 物理学 2021-02-17 Abigail J. Lee , Wendy L. Freedman , Barry F. Madore , Kayla A. Owens , Andrew J. Monson , Taylor J. Hoyt

Generic scalar-tensor theories of gravity predict deviations from Newtonian physics inside astrophysical bodies. In this paper, we point out that low mass stellar objects, red and brown dwarf stars, are excellent probes of these theories.…

宇宙学与河外天体物理 · 物理学 2017-12-12 Jeremy Sakstein

The tip of the red giant branch (TRGB) allows for the measurement of precise and accurate distances to nearby galaxies, based on the brightest ascent of low-mass red giant branch stars before they undergo the helium flash. With the advent…

Given the recent successful launch of the James Webb Space Telescope, determining robust calibrations of the slopes and absolute magnitudes of the near- to mid-infrared Tip of the Red Giant Branch (TRGB) will be essential to measuring…

星系天体物理 · 物理学 2023-11-10 Barry F. Madore , Wendy L. Freedman , Kayla Owens
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