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The two major approaches to studying macroevolution in deep time are the fossil record and reconstructed relationships among extant taxa from molecular data. Results based on one approach sometimes conflict with those based on the other,…

种群与进化 · 定量生物学 2018-04-02 Melanie J. Hopkins , David W. Bapst , Carl Simpson , Rachel C. M. Warnock

Recent methodological advances are enabling better examination of speciation and extinction processes and patterns. A major open question is the origin of large discrepancies in species number between groups of the same age. Existing…

种群与进化 · 定量生物学 2015-09-01 Sacha Laurent , Marc Robinson-Rechavi , Nicolas Salamin

Estimation of molecular evolutionary divergence times requires models of rate change. These vary with regard to the assumption of what quantity is penalized. The possibilities considered are the rate of evolution, the log of the rate of…

基因组学 · 定量生物学 2007-12-31 Peter J Waddell

Observations that rates of molecular evolution vary widely within and among lineages have cast doubts upon the existence of a single molecular clock. Differences in the timing of evolutionary events estimated from genetic and fossil…

种群与进化 · 定量生物学 2007-05-23 James F. Gillooly , Andrew P. Allen , Geoffrey B. West , James H. Brown

We address the emerging discrepancy between the Big Bang Nucleosynthesis data and standard cosmology, which asks for a bit longer evolution time. If this effect is real, one possible implication (in a framework of brane cosmology model) is…

高能物理 - 理论 · 物理学 2009-08-18 V. V. Flambaum , E. V. Shuryak

Unexplained annual variations in nuclear decay rates have been reported in recent years by a number of groups. We show that data from these experiments exhibit not only variations in time related to Earth-Sun distance, but also…

核实验 · 物理学 2011-06-09 Ephraim Fischbach , Jere H. Jenkins , Peter A. Sturrock

We assess the systematic uncertainties in stellar evolutionary calculations for low- to intermediate-mass, main-sequence stars. We compare published stellar tracks from several different evolution codes with our own tracks computed using…

太阳与恒星天体物理 · 物理学 2016-02-17 R. J. Stancliffe , L. Fossati , J. -C. Passy , F. R. N. Schneider

Divergence time estimation requires the reconciliation of two major sources of data. These are fossil and/or biogeographic evidence that give estimates of the absolute age of nodes (ancestors) and molecular estimates that give us estimates…

种群与进化 · 定量生物学 2008-12-31 Peter J Waddell

Many exoplanets have orbital characteristics quite different from those seen in our own solar system, including planets locked in orbital resonances and planets on orbits that are elliptical or highly inclined from their host star's spin…

地球与行星天体物理 · 物理学 2020-10-28 Emily D. Safsten , Rebekah I. Dawson , Angie Wolfgang

The recent distance determinations by HIPPARCOS have allowed to locate very precisely a reasonable set of subdwarfs in the HR diagram. A detailed comparison with evolutionary models is now possible and it has been recently claimed that the…

天体物理学 · 物理学 2007-05-23 P. Morel , A. Baglin

Globally disruptive events include asteroid/comet impacts, large igneous provinces and glaciations, all of which have been considered as contributors to mass extinctions. Understanding the overall relationship between the timings of the…

地球与行星天体物理 · 物理学 2016-04-15 Michael Gillman , Hilary Erenler

In certain pulsar timing experiments, where observations are scheduled approximately periodically (e.g. daily), timing models with significantly different frequencies (including but not limited to glitch models with different frequency…

高能天体物理现象 · 物理学 2021-04-28 Liam Dunn , Marcus E. Lower , Andrew Melatos

Correlations between planetary and stellar properties, particularly age, can provide insight on planetary formation and evolution processes. However, the underlying source of such trends can be unclear, and measurement uncertainties and…

地球与行星天体物理 · 物理学 2022-03-30 Emily D. Safsten , Rebekah I. Dawson

The expansion of deleted mitochondrial DNA (mtDNA) molecules has been linked to ageing, particularly in skeletal muscle fibres; its mechanism has remained unclear for three decades. Previous accounts assigned a replicative advantage to the…

种群与进化 · 定量生物学 2020-09-02 Ferdinando Insalata , Hanne Hoitzing , Juvid Aryaman , Nick S. Jones

Mutations can arise from the chance misincorporation of nucleotides during DNA replication or from DNA lesions that are not repaired correctly. We introduce a model that relates the source of mutations to their accumulation with cell…

种群与进化 · 定量生物学 2015-07-27 Ziyue Gao , Minyoung J. Wyman , Guy Sella , Molly Przeworski

Mitochondrial function relies on the coordinated expression of mitochondrial and nuclear genes, exhibiting remarkable resilience regardless the susceptibility of mitochondrial DNA (mtDNA) to accumulate harmful mutations. A suggested…

种群与进化 · 定量生物学 2024-10-16 Débora Princepe , Marcus A. M. de Aguiar

Several researchers have previously identified a severe climatic upheaval in tropical North Africa that began just over 4000 years ago and lasted for about three centuries. The upheaval is known to have occurred shortly after a volcanic…

地球物理 · 物理学 2007-05-23 Douglas J. Keenan

Asteroseismological determinations of stellar ages have shown that old main-sequence dwarfs do not obey gyrochronology. Their rotation is slow compared to young stars but faster than gyrochronology predicts. This can be explained by the…

太阳与恒星天体物理 · 物理学 2017-11-13 Leonid Kitchatinov , Alexander Nepomnyashchikh

A fundamental description of time can be consistent not only with the usual monotonic behavior but also with a periodic physical clock variable, coupled to the degrees of freedom of a system evolving in time. Generically, one would in fact…

量子物理 · 物理学 2022-05-25 Martin Bojowald , Luiz Martinez , Garrett Wendel

This is the second paper of a series which aims at quantifying the uncertainties in chemical evolution model predictions related to the underlying model assumptions. Specifically, it deals with the uncertainties due to the choice of the…

星系天体物理 · 物理学 2015-05-19 D. Romano , A. I. Karakas , M. Tosi , F. Matteucci
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