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  • Exam Code: H35-210_V2.5-ENU
  • Exam Name: HCIA-Access V2.5
  • Version: V17.95
  • Q & A: 400 Questions and Answers
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  • Exam Code: H35-210_V2.5-ENU
  • Exam Name: HCIA-Access V2.5
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  • Exam Code: H35-210_V2.5-ENU
  • Exam Name: HCIA-Access V2.5
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NEW QUESTION: 1
あなたの組織は最近Googleですか? 6ヶ月前。先週、ユーザーのGmailに新機能が登場しましたが、変更が行われていることを知らなかったため、CTOは驚いていました。 CTOは、新機能について積極的に更新したいと考えています。 CTOに情報を提供し続けるためのリアルタイム情報の最良の情報源は何ですか?
A. 四半期ごとのビジネスレビュー
B. GSuiteの四半期ロードマップ
C. クラウドコネクトコミュニティフォーラム
D. G SuiteUpdateブログ
Answer: D

NEW QUESTION: 2
The discoveries of the white dwarf, the neutron star, and the black hole, coming well after the discovery of the red giant are among eh most exciting developments in decades because they may be well present physicists with their greatest challenge since the failure of classical mechanics. In the life cycle of the star, after all of the hydrogen and helium fuel has been burned, the delicate balance between the outer nuclear radiations. Pressure and the stable gravitational force becomes disturbed and slow contraction begins. As compression increases, a very dense plasma forms. If the initial star had mass of less than 1.4 solar masses (1.4 times the mass of our sun), the process ceases at the density of 1,000 tons per cubic inch, and the star becomes the white dwarf. However, if the star was originally more massive, the white dwarf plasma can't resist the gravitations pressures, and in rapid collapse, all nuclei of the star are converted to a gas of free neutrons. Gravitational attraction compresses this neutron gas rapidly until a density of 10 tons per cubic inch is reached; at this point the strong nuclear force resists further contraction. If the mass of the star was between 1.4 and a few solar masses, the process stops here, and we have a neutron star. But if the original star was more massive than a few solar masses, even the strong nuclear forces cannot resist the gravitational brunch. The neutrons are forced into one another to form heavier hadrons and these in turn coalesce to form heavier entities, of which we as yet know nothing. At this point, a complete collapse of the stellar mass occurs; existing theories predict a collapse to infinite density and infinitely small dimensions Well before this, however, the surface gravitational force would become so strong that no signal could ever leave the star - any photon emitted would fall back under gravitational attraction - and the star would become black hole in space. This gravitational collapse poses a fundamental challenge to physics. When the most widely accepted theories predict such improbable things as infinite density and infinitely small dimensions, it simply means that we are missing some vital insight. This last happened in physics in the 1930's, when we faced the fundamental paradox concerning atomic structure. At that time, it was recognized that electrons moved in table orbits about nuclei in atoms. However, it was also recognized that if charge is accelerated, as it must be to remain in orbit, it radiates energy; so, theoretically, the electron would be expected eventually to spiral into the nucleus and destroy the atom.
Studies centered around this paradox led to the development of quantum mechanics. It may well be that an equivalent t advance awaits us in investigating the theoretical problems presented by the phenomenon of gravitational collapse.
The author asserts that the discoveries of the white dwarf, the neutron star, and the black hole are significant because these discoveries.
A. assist in establishing the age of the universe by tracing the life histories of stars.
B. clarify the paradox suggested by the collapse of electrons into atomic nuclei.
C. establish the relationship between the mass and gravitational pressure.
D. demonstrate the probability of infinite density and infinitely small dimensions.
E. pose the most comprehensive and fundamental problem faced by physicists in decades.
Answer: E
Explanation:
Explanation/Reference:
Explanation:

NEW QUESTION: 3
You are troubleshooting media issues during SIP calls on a C-series collaboration endpoint that is running TC6.3 software.
You are asked to recreate the problem and to provide a packet capture from the endpoint.
Which four of the following are required to accurately perform a packet capture on a C-series endpoint? (Choose four.)
A. Set the default transport to TCP.
B. Set up administrator access on the endpoint.
C. Set up root access on the endpoint.
D. Start the call, and then enter the tcpdump command string to begin the capture.
E. Stop the capture by pressing the key combination Ctrl + C.
F. Start the capture by entering the tcpdump command string and then start the call.
G. On the endpoint, set the default transport to TLS.
Answer: A,C,E,F

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