Along time ago, in a galaxy far, far away, electric charge had not yet been invented, and atoms were held together by gravitational forces. compute the bohr radius (a0) and the n = 5 to n = 4 transition energy (e5 − e4) in a gravitationally bound hydrogen atom.

i was thinking more like reflects green light, just not sure

answer: the correct answer is 1.

explanation: there are various process in which a radioactive nuclei decays:

1) alpha decay: in this process, a heavier nuclei decays into lighter nuclei by releasing alpha particle. the mass number is reduced by 4 units.

2) electron capture: in this decay process, a parent nuclei absorbs an electron and gets converted into a neutron. simply, a proton and an electron combines together to form a neutron. mass number does not change in this process.

3) gamma ray emission: it is a decay process in which an unstable nuclei gives excess energy by a spontaneous electromagnetic process. this decay releases . this process does not change the mass number.

4) positron emission: it is a type of decay process, in which a proton gets converted to neutron and an electron neutrino. this is also known as -decay. in this the mass number remains same.

from the above information, we see that only alpha-decay is producing a change in the mass number of the nucleus.

explanation:

v=uf/(u-f)

= 5.-10/(5+10) convex lens has negative focal length