scholarly journals Cosmographic Evaluation of the Deceleration Parameter Using Type Ia Supernova Data

2004 ◽  
Vol 614 (1) ◽  
pp. 1-5 ◽  
Author(s):  
Moncy V. John
2013 ◽  
Vol 22 (09) ◽  
pp. 1350060 ◽  
Author(s):  
WEN ZHAO ◽  
PUXUN WU ◽  
YANG ZHANG

In this paper, we study the anisotropy of cosmic acceleration by dividing the Union2 Type Ia supernova (SNIa) dataset into 12 subsets according to their positions in Galactic coordinate system. In each region, we derive the deceleration parameter q0 as the diagnostic to quantify the anisotropy level in the corresponding direction, and construct q0 anisotropic maps by combining these q0 values. In addition to the monopole component, we find the significant dipole effect in the q0-maps with the amplitude [Formula: see text], which deviates from zero at more than 2-σ level. The direction of the best-fit dipole is (θ = 108.8°, ϕ = 187.0°) in Galactic system. Interesting enough, we find the direction of this dipole is nearly perpendicular to the CMB kinematic dipole, and the angle between them is 95.7°. The perpendicular relation is anomalous at the 1-in-10 level.


1999 ◽  
Vol 514 (2) ◽  
pp. 844-855 ◽  
Author(s):  
A. Finoguenov ◽  
C. Jones ◽  
W. Forman ◽  
L. David

2009 ◽  
Vol 697 (1) ◽  
pp. 380-408 ◽  
Author(s):  
X. Wang ◽  
W. Li ◽  
A. V. Filippenko ◽  
R. J. Foley ◽  
R. P. Kirshner ◽  
...  

2010 ◽  
Vol 410 (1) ◽  
pp. 585-611 ◽  
Author(s):  
Jeffrey M. Silverman ◽  
Mohan Ganeshalingam ◽  
Weidong Li ◽  
Alexei V. Filippenko ◽  
Adam A. Miller ◽  
...  
Keyword(s):  
Type Ia ◽  

2016 ◽  
Vol 466 (1) ◽  
pp. 884-891 ◽  
Author(s):  
David Cinabro ◽  
Daniel Scolnic ◽  
Richard Kessler ◽  
Ashley Li ◽  
Jake Miller
Keyword(s):  

2011 ◽  
Vol 63 (4) ◽  
pp. L31-L35 ◽  
Author(s):  
Xiang Cun Meng ◽  
Zhong Mu Li ◽  
Wu Ming Yang

2006 ◽  
Vol 2 (14) ◽  
pp. 308-309
Author(s):  
Friedrich K. Röpke

AbstractKeeping up with ever more detailed observations, Type Ia supernova (SN Ia) explosion models have seen a brisk development over the past years. The aim is to construct a self-consistent picture of the physical processes in order to gain the predictive power necessary to answer questions arising from the application of SNe Ia as cosmological distance indicators. We review recent developments in modeling these objects focusing on three-dimensional simulations.


2011 ◽  
Vol 745 (1) ◽  
pp. 75 ◽  
Author(s):  
D. García-Senz ◽  
C. Badenes ◽  
N. Serichol

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