نتایج جستجو برای: d plot of yp

تعداد نتایج: 21225361  

Journal: :Journal of medical genetics 2005
A Sharp K Kusz J Jaruzelska W Tapper M Szarras-Czapnik J Wolski P Jacobs

D uring male meiosis the X and Y chromosomes pair along much of their length, with a single obligatory recombination event usually occurring in the pseudoautosomal region (PAR) at the tip of Xp and Yp, thus maintaining identity of the sex chromosome PARs. Occasionally illegitimate crossover occurs outside the PAR, resulting in the transfer of Y specific sequences onto the X chromosome. Such tra...

2005
A Sharp K Kusz J Jaruzelska W Tapper M Szarras-Czapnik J Wolski P Jacobs

D uring male meiosis the X and Y chromosomes pair along much of their length, with a single obligatory recombination event usually occurring in the pseudoautosomal region (PAR) at the tip of Xp and Yp, thus maintaining identity of the sex chromosome PARs. Occasionally illegitimate crossover occurs outside the PAR, resulting in the transfer of Y specific sequences onto the X chromosome. Such tra...

2013
M Byrd S Simbo YP Jung B Sanchez M Cho CW Lee B Lockard C Baetge K Levers E Galvan A Jagim JM Oliver R Dalton B Bessire K Horrell T Leopold M Koozehchian D Khanna K Shimkus W Gapinsky M Perez J Hart S Riechman J Fluckey M Greenwood C Rasmussen R Kreider

Effects of immediate and delayed nutrient timing following resistance exercise on changes in mixed muscle fractional synthesis rate (FSR) in post-menopausal women participating in a weight loss program M Byrd, S Simbo, YP Jung, B Sanchez, M Cho, CW Lee, B Lockard, C Baetge, K Levers, E Galvan, A Jagim, JM Oliver, R Dalton, B Bessire, K Horrell, T Leopold, M Koozehchian, D Khanna, K Shimkus, W G...

2008
Kazuhide Ichikawa Tomo Takahashi

We revisit the constraint on the primordial helium mass fraction Yp from observations of cosmic microwave background (CMB) alone. By minimizing χ of recent CMB experiments over 6 other cosmological parameters, we obtained rather weak constraints as 0.17 ≤ Yp ≤ 0.52 at 1σ C.L. for a particular data set. We also study the future constraint on cosmological parameters when we take account of the pr...

2001
Rune Dalgaard

W ith th e W eb , h y per text h as b ecom e the p ar ad igm atic r h eto rical s tr u ctu r e o f a g lo bal and d istr ibu ted ar ch iv e. Th is pap er ar g ues that th e s ch o lar ly ar ch iv e is g o ing tho u g h a p r ocess o f h y p ertextu alization that is n o t ad eq uately acco u n ted f o r in th eo r ies on h y per text. A m eth od o log ical ap p ro ach b ased o n G er ar d Gen e...

Journal: :Universe 2023

We explore the effect of neutron lifetime and its uncertainty on standard big bang nucleosynthesis (BBN). BBN describes cosmic production light nuclides, 1H, D, 3H+3He, 4He, 7Li+7Be, in first minutes time. The mean life τn has two roles modern calculations: (1) it normalizes matrix element for weak n↔p interconversions, (2) sets rate free decay after interactions freeze-out. review history inte...

2002
V. LURIDIANA

The primordial abundance of He, YP , is one of the hottest themes in present-day astronomy, mostly due to its cosmological relevance. The disagreement between different determinations has been currently reduced to the 1-2% level, but these differences are still large enough to have deep implications for Big-Bang nucleosynthesis. It is therefore crucial to estimate precisely the uncertainties in...

Journal: :Electr. Notes Theor. Comput. Sci. 2002
Stephen L. Bloom Zoltán Ésik

x1 = t1(x1, . . . , xn, y1, . . . yp) .. (1) xn = tn(x1, . . . , xn, y1, . . . yp), where, typically, for each i ∈ [n], ti denotes a function ti : A → A, for some structure A. Sometimes, the structure A is equipped with a partial order, and the functions ti are order-preserving or continuous. In such a case, for a given p-tuple of elements y1, . . . , yp in A, one might ask for the least x1, . ...

2006
Kazuhide Ichikawa Tomo Takahashi

We revisit the constraint on the primordial helium mass fraction Yp from observations of cosmic microwave background (CMB) alone. By minimizing χ of recent CMB experiments over 6 other cosmological parameters, we obtained rather weak constraints as 0.17 ≤ Yp ≤ 0.52 at 1σ C.L. for a particular data set. We also study the future constraint on cosmological parameters when we take account of the pr...

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