The proton is a composite particle composed of three quarks, all of which are either up quarks (u; charge +
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- Considering electron and proton as two charged particles separated by d = 5.9 × 10-11 m calculate the gravitational force between the proton and electron and find its ratio to the Coulomb force. Take the mass of the proton 1.7 x 10-27 kg, the mass of the electron 9.1 x 10-31 kg, the value of = 9x10⁹ m/F. Give the answer for the universal gravitational constant 6.7 x 10-11 N kg 2m-2, the electron charge -1.6 x 10-¹9 C and the gravitational force in 10-47 N. 1 Απερ Answer:arrow_forwardThe quark compositions of the proton and neutron are, respectively, uud and udd, where u is an up quark (charge + 23 e2 and d is a down quark (charge - 13 e2. There are also antiup u (charge - 23 e2 and antidown d (charge + 13 e2 quarks. The combination of a quark and an antiquark is called a meson. The mesons known as pions have the composition p+ = ud and p- = ud. Suppose a proton collides with an antineutron. During such collisions, the various quarks and antiquarks annihilate whenever possible. When the remaining quarks combine to form a single particle, it is aA. Proton B. Neutron C. p+ D. parrow_forwardConsidering electron and proton as two charged particles separated by d = 5.7 × 10-11 m calculate the gravitational force between the proton and electron and find its ratio to the Coulomb force. Take the mass of the proton 1.7 × 10¬2 kg, the mass of the electron 9.1 × 10¬3' kg, the value of the universal 1 = 9 x 10° m/F. Give the answer for the gravitational force in 10" gravitational constant 6.7 x 10-11 N kg?m² , the electron charge –1.6 × 10-19 c and 4πεο 47 N.arrow_forward
- A synchrotron of 25 m radius accelerates protons from a kinetic energy of 50 to 1000 MeV in 1 second. The dipole magnets saturate at 1000 MeV. i) What is the maximal kinetic energy of a deuteron that it could accelerate? ii) Calculate the revolution frequency for protons and deuterons.arrow_forwardConsider (Figure 1) showing a proton approaching a helium-3 nucleus that has two protons and one neutron. Figure 1 of 1 Proton Helium-3 nucleus Initial 9= +2e Зт 9 = +e m To = 0 v = 0 Final (the proton is at rest)arrow_forwardAs a multiple of e1 what is the charge q1 of the particle that is composed of the quark combination udd? q1 = ? e As a multiple of e1 what is the charge q2 of the particle that is composed of the quark combination dds? q2 = ? earrow_forward
- 7636Kr + 0-1e → ? a) it is n (mass # : 1; charge:0) b) no right answer c) it is Br (mass # : 76; protons: 35) d) it is C (mass #: 14; protons 6) e) it is e ( mass #: 0 ; charge +1)arrow_forwardA cyclotron used to accelerate protons has a maximum radius of 0.4 m and the magnetic induction used is one tesla. Find the frequency of oscillator connected to the dees and the maximum velocity of emerging protons. Through what P.D. must the protons be accelerated from rest to achieve this speed? If deuterons are used instead of protons, what would be their final energy? Mp= 1.67 x 10-27 kg.arrow_forwardConsider an object of mass 48.8 kg. Assume that it s made up of equal numbers of protons, neutrons, and electrons. How many protons does this object contain? 5.84E+28 7.30E+27 1.46E+28 2.92E+28arrow_forward
- During most of its lifetime, a star maintains an equilibrium size in which the inward force of gravity on each atom is balanced by an outward pressure force due to the heat of the nuclear reactions in the core. But after all the hydrogen "fuel" is consumed by nuclear fusion, the pressure force drops and the star undergoes a gravitational collapse until it becomes a neutron star. In a neutron star, the electrons and protons of the atoms are squeezed together by gravity until they fuse into neutrons. Neutron stars spin very rapidly and emit intense pulses of radio and light waves, one pulse per rotation. These "pulsing stars" were discovered in the 1960s and are called pulsars. Part A A star with the mass (M = 2.0 × 10³0 kg) and size (R = 3.5 × 108 m) of our sun rotates once every 33.0 days. After undergoing gravitational collapse, the star forms a pulsar that is observed by astronomers to emit radio pulses every 0.200 s. By treating the neutron star as a solid sphere, deduce its radius.…arrow_forwardDuring most of its lifetime, a star maintains an equilibrium size in which the inward force of gravity on each atom is balanced by an outward pressure force due to the heat of the nuclear reactions in the core. But after all the hydrogen "fuel" is consumed by nuclear fusion, the pressure force drops and the star undergoes a gravitational collapse until it becomes a neutron star. In a neutron star, the electrons and protons of the atoms are squeezed together by gravity until they fuse into neutrons. Neutron stars spin very rapidly and emit intense pulses of radio and light waves, one pulse per rotation. These "pulsing stars" were discovered in the 1960s and are called pulsars. A star with the mass (M=2.0×10^30kg) and size (R=3.5×10^8m) of our sun rotates once every 29.0 days. After undergoing gravitational collapse, the star forms a pulsar that is observed by astronomers to emit radio pulses every 0.200 s. By treating the neutron star as a solid sphere, deduce its radius.arrow_forwardDuring most of its lifetime, a star maintains an equilibrium size in which the inward force of gravity on each atom is balanced by an outward pressure force due to the heat of the nuclear reactions in the core. But after all the hydrogen "fuel" is consumed by nuclear fusion, the pressure force drops and the star undergoes a gravitational collapse until it becomes a neutron star. In a neutron star, the electrons and protons of the atoms are squeezed together by gravity until they fuse into neutrons. Neutron stars spin very rapidly and emit intense pulses of radio and light waves, one pulse per rotation. These "pulsing stars" were discovered in the 1960s and are called pulsars. A star with the mass (m=2.0×10^30kg) and size (R=3.5×10^8m) of our sun rotates once every 35.0 days. After undergoing gravitational collapse, the star forms a pulsar that is observed by astronomers to emit radio pulses every 0.200 s. By treating the neutron star as a solid sphere, deduce its radius. What is the…arrow_forward
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