The stems contain a quantity of fibrous matter, which makes excellent rope.
"The Young Berringtons" by W.H.G. Kingston
Besides, the name is a comprehensive one, and should include a quantity of fine matter.
"The Letters of Charles Dickens" by Charles Dickens
What important matter could have brought so many men on to the deck of the frigate, bearing with them quantities of fruits and figs?
"Celebrated Travels and Travellers" by Jules Verne
The effect of its application is to lessen the total quantity of dry matter and sugar in the plant.
"Manures and the principles of manuring" by Charles Morton Aikman
Except that he saw two patients, who recovered after discharging a large quantity of matter at the navel.
"Zoonomia, Vol. II" by Erasmus Darwin
If you use good judgment both as to the quality and quantity of foods, you need then give the matter very little thought.
"What a Young Woman Ought to Know" by Mary Wood-Allen
One was to boil a quantity of ground coffee to get a maximum of body or soluble matter.
"All About Coffee" by William H. Ukers
We have never seen a volume embracing any thing like the same quantity of useful matter.
"The Humors of Falconbridge" by Jonathan F. Kelley
I soon learned that these alluring reports should be taken with the usual quantity of saline matter.
"Confessions of a Neurasthenic" by William Taylor Marrs
The fermentable matter, such as sugar, with a proper quantity of yeast, and diluted with water, is put into the matrass.
"Elements of Chemistry," by Antoine Lavoisier
This comparison was once applied to herself by George Sand, Zola's only rival in the matter of quantity.
"Ivory Apes and Peacocks" by James Huneker
A small quantity of prepared matter occasions a terrible explosion accompanied by a brilliant light.
"The Popes and Science" by James J. Walsh
Nor was it only a matter of quantity, but a matter of quality also.
"A Historical Geography of the British Colonies" by Charles Prestwood Lucas
Into these furrows the gray matter of the surface is extended, and, in this manner, its quantity is vastly increased.
"A Treatise on Physiology and Hygiene" by Joseph Chrisman Hutchison
Now until I know the quantity of matter requisite for one I cannot effect this.
"Charles Lever, His Life in His Letters, Vol. I (of II)" by Edmund Downey
Charles James Lever
Violent purging soon terminates the disease, death being generally preceded by the evacuation of a quantity of blackish matter.
"A Treatise on Sheep:" by Ambrose Blacklock
Now, the force of gravity in a body is greater, in proportion as its quantity of matter is greater.
"Letters on Astronomy" by Denison Olmsted
The skin is very red, and covered with down and a considerable quantity of sebaceous matter.
"Private Sex Advice to Women" by R. B. Armitage
These critical notes often nearly equalled in quantity of matter the original text.
"Genius in Sunshine and Shadow" by Maturin Murray Ballou
They dispose of vast quantities of carrion and other offensive matter.
"The Children's Book of Birds" by Olive Thorne Miller
The density ﬂuctuation is deﬁned by δ = (ρ − ¯ρ)/ ¯ρ for each component of matter where the quantities with bar denotes the background quantity.
Consistency test of general relativity from large scale structure of the Universe
The components of the state vector are gauge invariant metric and matter perturbation quantities.
Report on GRG18, Session A3, Mathematical Studies of the Field Equations
The quantities P 0 = q0 + EN (~p) and ~P = ~q + ~p are the total energy and momentum of the DN pair in the nuclear matter rest frame, with EN (~p ) being the single-particle nucleon energy and the values (q0, ~q ) the energy and momentum of the D meson also in this frame.
Charm and hidden charm scalar mesons in the nuclear medium
Because the tests we are presenting require the use of pro jected quantities, we will focus in particular on how those artifacts affect the pro jected galaxy distribution within a redshift bin in its comparison to the pro jected matter distribution.
A step towards testing general relativity using weak gravitational lensing and redshift surveys
There have been many efforts in last two decades using various observations to distinguish between cosmological models and put constraints on some of the key cosmological quantities like matter density, curvature and dark energy.
Testing cosmological models using relative mass-redshift abundance of SZ clusters
Therefore the study of this quantity M ≡ dµ/dn is of high importance in condensed matter physics and is the principal sub ject which we will address in this review.
The compressibility of graphene
In Figs. 10a - 10d, we plot the quantity E 2 × dΦ dE for different values E, the energy of the emitted γ rays from dark matter annihilations.
Gamma Ray and Neutrino Flux from Annihilation of Neutralino Dark Matter at Galactic Halo Region in mAMSB Model
Since only very small quantities of non-baryonic dark matter is present in disks, the dark component of collisional debris should be dark baryons.
What collisional debris can tell us about galaxies
Indeed, it is a matter of fact that when experimenters measure a physical quantity in the laboratory, on a quantum system, what they do is precisely to repeat the same experiment a large number of times, on identically prepared systems, in order to calculate probabilities as limits of relative frequencies of outcomes.
Only in models with large dark energy perturbations or modiﬁcations of Einstein gravity, the two quantities might be different, and special care about the deﬁnition of the matter power spectrum is needed.
TASI Lectures on Cosmological Perturbations
In the 90’s, the ﬁrst estimates of the matter power spectrum P (k) (or of some related quantities) on galaxy scales and cluster scales showed clearly that the HDM scenario was ruled out.
TASI Lectures on Cosmological Perturbations
Similar ratios were obtained from the virial theorem for the centers of other rich clusters indicating the existence of large quantities of gravitating dark matter in rich clusters of galaxies.
Tests of General Relativity at Large Distances and Dark Matter -
The quantity of dark matter on different scales is quoted using Ω = ρ/ρcrit, where ρ is the density of some material averaged over the Universe, and ρcrit is the critical density.
The Particle- and Astro-Physics of Dark Matter
Both of these quantities have their origin in the mixing of semi-classical gravity and matter in the tunneling region.
Time and Entropy from Semi-classical Tunneling of the Cosmological Scale Function
Wilson has proposed evolving the system through a sequence of initial-value problems by solving the full dynamical equations for the matter in the instantaneous background metric, and then updating the metric quantities at each time step by re-solving the selected subset of Einstein’s equations.
Testing a Simplified Version of Einstein's Equations for Numerical Relativity