Oscillation Modes of Strange Quark Stars with a Strangelet Crust
... Next we compute the f and p modes for a homogeneous quark star having an EOS defined as in Eq. 1, and study their dependence on the stellar mass. The mass of the strange quark, the value of the critical quark chemical potential, and the interaction parameters a4 are tunable features in the equation ...
... Next we compute the f and p modes for a homogeneous quark star having an EOS defined as in Eq. 1, and study their dependence on the stellar mass. The mass of the strange quark, the value of the critical quark chemical potential, and the interaction parameters a4 are tunable features in the equation ...
RESEARCH STATEMENT Chromospheres and winds
... been observed in the optical using ground–based instruments [2] and in the ultraviolet using the International Ultraviolet Explorer (IUE) [3]. ζ Aurigae has been observed at the Dominion Astronomical Observatory (DAO) over many eclipse cycles with the 1.2 m telescope. The chromospheric Ca ii K absor ...
... been observed in the optical using ground–based instruments [2] and in the ultraviolet using the International Ultraviolet Explorer (IUE) [3]. ζ Aurigae has been observed at the Dominion Astronomical Observatory (DAO) over many eclipse cycles with the 1.2 m telescope. The chromospheric Ca ii K absor ...
Toward $ ab\, initio $ extremely metal poor stars
... Smith et al. 2009). In comparison, the critical metallicity above which dust can explain the formation of the known metal-poor stars is Zcrit,dust ∼ 10−6 Z , assuming a reference fraction of metal mass depleted in dust of fdust = 0.22 − 0.24 (Schneider et al. 2006, 2012, see, also, Omukai, Hosokawa ...
... Smith et al. 2009). In comparison, the critical metallicity above which dust can explain the formation of the known metal-poor stars is Zcrit,dust ∼ 10−6 Z , assuming a reference fraction of metal mass depleted in dust of fdust = 0.22 − 0.24 (Schneider et al. 2006, 2012, see, also, Omukai, Hosokawa ...
Chapter 9 MOTION IN FIELDS
... We have seen that if we lit an object of mass m to a height h above the surface of the Earth then its gain in gravitational potential energy is mgh. However, this is by no means the full story. For a start we now know that g varies with h and also the expression really gives a diference in potential ...
... We have seen that if we lit an object of mass m to a height h above the surface of the Earth then its gain in gravitational potential energy is mgh. However, this is by no means the full story. For a start we now know that g varies with h and also the expression really gives a diference in potential ...
Near Surface Geophysics Glossary
... designated as 0 or 1; in drilling: the end of the drill assembly that cuts the rock In seismic refraction survey: an interface which does not show up as a first arrival at any source-receiver offset due to its small thickness and a seismic wave velocity which is insufficiently greater than the under ...
... designated as 0 or 1; in drilling: the end of the drill assembly that cuts the rock In seismic refraction survey: an interface which does not show up as a first arrival at any source-receiver offset due to its small thickness and a seismic wave velocity which is insufficiently greater than the under ...
7. Paradise Gravity
... Absolute gravity is a long-range interaction between individual ultimatons and the Isle of Paradise, which has “a potential infinity of gravity extension.” 11:8.9 Unlike other later forms of materialization evolved from cosmic force, ultimatons do not gravitationally interact with other ultimatons ...
... Absolute gravity is a long-range interaction between individual ultimatons and the Isle of Paradise, which has “a potential infinity of gravity extension.” 11:8.9 Unlike other later forms of materialization evolved from cosmic force, ultimatons do not gravitationally interact with other ultimatons ...
Physics 100
... A meter stick is limited by the size of its smallest division (0.1 cm). Vernier calipers, on the other hand, can be used to make much more precise measurements. However, with most increases in precision comes a limitation. In the case of the calipers their maximum range of measurement is about 20 cm ...
... A meter stick is limited by the size of its smallest division (0.1 cm). Vernier calipers, on the other hand, can be used to make much more precise measurements. However, with most increases in precision comes a limitation. In the case of the calipers their maximum range of measurement is about 20 cm ...
M060056-07 - LIGO dcc - LIGO Scientific Collaboration
... limitations. To define the goal sensitivity of Advanced LIGO, a single measure is given: a equivalent strain noise of 10-22 RMS, integrated over a 100 Hz bandwidth centered at the minimum noise region of the strain spectral density, a factor of 10 more sensitive than initial LIGO. This measure allow ...
... limitations. To define the goal sensitivity of Advanced LIGO, a single measure is given: a equivalent strain noise of 10-22 RMS, integrated over a 100 Hz bandwidth centered at the minimum noise region of the strain spectral density, a factor of 10 more sensitive than initial LIGO. This measure allow ...
Electrogravitics Systems - Reports On a New Propulsion Methodology
... Let us re-examine Brown's works and rethink some of the issues which he has suggested to us. Science is an ongoing process, not a fixed set of facts, ever changing and developing. ...
... Let us re-examine Brown's works and rethink some of the issues which he has suggested to us. Science is an ongoing process, not a fixed set of facts, ever changing and developing. ...
Anglická verze kvartonovky
... made up of a solid or liquid material substance, coated with something so rare, that through it some how it can comfortably walk. And all this, apparently freely, lying around 'in bleak empty space, in short, like ‚Something' in Nothing. Physics (except inflamed éteristů) course primarily interested ...
... made up of a solid or liquid material substance, coated with something so rare, that through it some how it can comfortably walk. And all this, apparently freely, lying around 'in bleak empty space, in short, like ‚Something' in Nothing. Physics (except inflamed éteristů) course primarily interested ...
Paper 25 - Free-Energy Devices
... Let us re-examine Brown's works and rethink some of the issues which he has suggested to us. Science is an ongoing process, not a fixed set of facts, ever changing and developing. ...
... Let us re-examine Brown's works and rethink some of the issues which he has suggested to us. Science is an ongoing process, not a fixed set of facts, ever changing and developing. ...
Characteristics of nighttime medium
... and horizontal lines near the southern edge of the images are caused by the Moon. structure appearance time is equivalent to 1630–1930 LT on the evening of the preceding day. [12] Figure 3 (top) shows two‐dimensional distributions of O I 630.0 nm emissions intensity projected on the map of Alaska an ...
... and horizontal lines near the southern edge of the images are caused by the Moon. structure appearance time is equivalent to 1630–1930 LT on the evening of the preceding day. [12] Figure 3 (top) shows two‐dimensional distributions of O I 630.0 nm emissions intensity projected on the map of Alaska an ...
Gamma-ray emission from Wolf
... deserve further study in the light of the most recent observations. This is particularly true for WR 140, a very interesting system whose possible high-energy emission has been already discussed in the pre-EGRET era by Pollock (1987) and also by Eichler & Usov (1993) in their seminal paper on non-th ...
... deserve further study in the light of the most recent observations. This is particularly true for WR 140, a very interesting system whose possible high-energy emission has been already discussed in the pre-EGRET era by Pollock (1987) and also by Eichler & Usov (1993) in their seminal paper on non-th ...
the first simultaneous microlensing observations by two space
... provides supporting evidence for a conclusion previously drawn from microlensing studies: that BDs around main sequence stars are relatively common at separations of a few au (Shvartzvald et al. 2016) as compared with their rarity at closer separations according to radial-velocity studies (e.g., Gre ...
... provides supporting evidence for a conclusion previously drawn from microlensing studies: that BDs around main sequence stars are relatively common at separations of a few au (Shvartzvald et al. 2016) as compared with their rarity at closer separations according to radial-velocity studies (e.g., Gre ...