Fill in the information missing from this table: subshell 1s 3d 2p Some electron subshells principal quantum number n 0 П 0 angular momentum quantum number / U maximum number of electrons 0 П 0 X 5

Which of the following electronic transitions is allowed and thus expected to have a short lifetime? 3S --> 1P 3S --> 3D 3S --> 3P 3S --> 1F

what is the absolute energy (wavenumbers) for hydrogn from n=6 to n=1

Hi I need help on one of my physical chemistry questions and I don't know how to do it. Will you please help me solve for it thank you very much!

Please answer both questions!! Please make sure it's handwritten and legible!!!

Which of the subshells below do not exist due to the constraints upon the angular momentum quantum number? A 2d 2s All of these D None of these E 2p

5. (McQuarrie 9-25) Show that the atomic determinantal wave function, 1 1sa (1) 1sẞ(1) V(r1, r2)= √2 1sa (2) 1sẞ(2) is normalized when the 1s orbitals are normalized. Hint: Don't freak out about this problem-it's easier than it looks! Expand the Slater determinant to get the wavefunction in a more usable form, then set up the normalization integral for . Multiply everything out, and you should have complicated-looking integrals such as this: (1sa (1) 1sẞ(2) | 1sa(1) 1sẞ(2)) While such integrals might look scary, they're actually straightforward. An integral like the one above has four pieces: integration over (a) the spatial coordinates of electron 1, (b) the spatial coordinates of electron 2, (c) the spin coordinates of electron 1, and (d) the spin coordinates of electron 2. You can break up these multi-dimensional integrals into separate integrals for each piece. For example: (1sa (1) 1sẞ(2) | 1sa(1) 1sẞ(2) ) = (1s(1)|1s(1)) · (a(1)|a(1)) · (1s(2)|1s(2)) · (6(2)|ß(2)) Then you can…

A hydrogen atom is immersed in a magnetic field so that its energy levels split according to the Zeeman effect. Neglecting any effects due to electron spin, how many unique energy levels are available to an electron in the 5f subshell?

3. Verify that the wave function p(x) = Ae-[(ku)¹/² x²/(zh)] (where 4. m. and kare A, m, all constants) is a solution to the Schrodinger equation ħ² d² 1-2 u |- ²2μ dx² + ½kx²] p(x) = Eq(x), and find the energy in terms of m, and k. j 2 horva Guation BossMabay

The wavefunction for the 2s orbital of a hydrogen atom is N((2-r)/a0)e-r/2a0. Evaluate the normalization constant N.