The Biggest Ideas in the Universe | 17. Matter

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  • เผยแพร่เมื่อ 13 ก.ค. 2020
  • The Biggest Ideas in the Universe is a series of videos where I talk informally about some of the fundamental concepts that help us understand our natural world. Exceedingly casual, not overly polished, and meant for absolutely everybody.
    This is Idea #17, "Matter." The matter of which we are made can be solid because electrons are fermions, meaning that they take up space. We talk about that and the closely related spin-statistics theorem. Complete with demonstrations using visual aids!
    My web page: www.preposterousuniverse.com/
    My TH-cam channel: / seancarroll
    Mindscape podcast: www.preposterousuniverse.com/p...
    The Biggest Ideas playlist: • The Biggest Ideas in t...
    Blog posts for the series: www.preposterousuniverse.com/b...
    Background image: www.publicdomainpictures.net/...
    #science #physics #ideas #universe #learning #cosmology #philosophy #matter #fermions #spin
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ความคิดเห็น • 222

  • @ofridagan
    @ofridagan 3 ปีที่แล้ว +9

    This series is going to be one of the most meaningful treasures of the world-wide-web.
    I wish some day humanity reach a point where everyone have a basic grasp on reality. These videos will definitely help get there!
    Truly a gift. Thank you.

  • @atl123
    @atl123 ปีที่แล้ว +1

    "...just be inspired by it, don't lean on it in times of trouble ..." may be my favourite quote ever. But these talks are, for certain, my favourite series of physics lectures/talks ever.

  • @ticklemeandillhurtyou5800
    @ticklemeandillhurtyou5800 3 ปีที่แล้ว +111

    Honestly I wish this would never end its kind of addicting

    • @ericsvilpis1635
      @ericsvilpis1635 3 ปีที่แล้ว +1

      tickle me and I'll Hurt you Only kind of??

    • @Canard712
      @Canard712 ปีที่แล้ว

      Rewind & replay.

  • @BertrandLeRoy
    @BertrandLeRoy 3 ปีที่แล้ว +4

    Sean, thank you for that explanation of spin as the angular momentum of the quantum field and for the discussion of spin zero, integer and fractional in the context of Noether’s conserved quantities. It has never been explained so clearly to me before, despite having a PhD in theoretical physics. What I like the most about this series is how it never takes the shut up and calculate road that so many professors take, and instead takes the time to explain what it all means, and calls out common shortcuts as inaccurate.

  • @nujuat
    @nujuat 3 ปีที่แล้ว +68

    Once again.
    Me: I’m going to bed now.
    Sean Carroll: Uploaded 3 minutes ago
    Me: new plan

    • @navidazadi4280
      @navidazadi4280 3 ปีที่แล้ว +3

      And we must thank him immediately, because such a cultured person and great scientist takes his time and does a great attention and service to our understanding of the world and physics and truth. Thank you very much dear Sean.
      (I'm a human being somewhere on an earth in a galaxy in this world )

    • @Kage1128
      @Kage1128 3 ปีที่แล้ว +1

      Go to bed and watch tomorrow its not worth messing up your sleeping schedule

    • @edithseichter4857
      @edithseichter4857 3 ปีที่แล้ว

      Try to go to bed at the same time every day and sleep at least 8 hours. Care for your health.

  • @albertfeuerstein8773
    @albertfeuerstein8773 3 ปีที่แล้ว +11

    Prof. Carroll, you are an extremely gifted teacher!
    Thank you so much for all your effort to put this series together.

  • @rc5989
    @rc5989 3 ปีที่แล้ว +6

    This is the best video on spin I have ever seen, and it’s not even close. Amazingly, Sean Carroll is using earlier Biggest Ideas to teach us later Biggest Ideas.
    This is a lot of hard work given freely and I am equally excited and grateful to Sean Carroll.

  • @etienga
    @etienga 3 ปีที่แล้ว +1

    That spin 1/2 practical example... got me on the edge of my seat. You can totally sense the Feynman of it.

  • @nujuat
    @nujuat 3 ปีที่แล้ว +13

    “So the Universe does ultimately make sense, if not only for the reasons you might initially have guessed.”
    Amazing

  • @ba0cbmft
    @ba0cbmft 3 ปีที่แล้ว +13

    Best explanation for spin I have ever found. Thank-you!

  • @barissannan2731
    @barissannan2731 3 ปีที่แล้ว +8

    its a great pleasure listening to all that complicated stuff so beautifully brought down to earth. Thanks a lot.

  • @ErnestGWilsonII
    @ErnestGWilsonII 3 ปีที่แล้ว +3

    First let me say thank you very much for making this video series and sharing it with all of us. I realize this series cannot go on forever, I hope you can find time to do another series after this series. A few thoughts, if our species goes to Mars for any reason, this series should come along for the ride and be part of the archive of things we would like to have saved (backed up) on a different planet. Additionally, it has been an extreme pleasure to have access to one of the greatest minds on Earth. It is particularly rewarding and enjoyable to have Sean Carroll reading comments, following up and doing Q&A videos as part of this series. I am grateful to be able to watch this series as it progresses. This series and or one like it hosted by Sean Carrol would be on national television picked up by a major network if I had my wish. The content is fantastic, the delivery is perfect, the interaction is excellent. I am of course subscribed to this TH-cam channel with notifications turned on and thumbs up!

  • @dougg1075
    @dougg1075 3 ปีที่แล้ว +16

    “ fieldness makes up nature “ that should smoke everybody’s minds

    • @mobaby1979
      @mobaby1979 3 ปีที่แล้ว

      It did mine!! It's a neat and weird fact. I definitely feel more cozy in a world made up of 'nature-ness' compared to fieldness

    • @whynottalklikeapirat
      @whynottalklikeapirat 3 ปีที่แล้ว

      @@mobaby1979 My head is full of "WHAT??!!o.O-ness"

  • @rhondagoodloe3275
    @rhondagoodloe3275 3 ปีที่แล้ว +12

    Sean, Thanks for your enthusiasm and patience in sharing your knowledge!

  • @paulc96
    @paulc96 3 ปีที่แล้ว +2

    Just got home and found a new BIitU video waiting. Ditto to Joao below - stop everything else. Get comfortable with a drink & a smoke - click on "Like" and starting watching for first time. Then watch again tomorrow, Brilliant. Thanks again Prof. Carroll.

  • @barefootalien
    @barefootalien 3 ปีที่แล้ว +2

    lol you just made my day, Sean! "Bosons vs. Fermions, that Classificashon..." XD
    Usually when you write and talk at the same time, it's the writing that dies a horrible death, but this time it was the talking, and I adore it!

  • @Ryo-sd9rx
    @Ryo-sd9rx ปีที่แล้ว

    You know what I love about physics is that you almost gain a sort of x-ray vision in a way, you see through things.

  • @markweitzman
    @markweitzman 3 ปีที่แล้ว +20

    @Professor Carroll, Sean you are so productive - its makes the rest of us look so lame :-).

    • @stephenbryant7873
      @stephenbryant7873 3 ปีที่แล้ว +2

      If you are watching the 33rd lecture in this series, I doubt you're an ineffective person in your area of expertise.

  • @DeezNutz-yg8io
    @DeezNutz-yg8io 3 ปีที่แล้ว +7

    Discussion of spin around minute 35 is one of the clearest I have heard!

  • @spiritmonarch
    @spiritmonarch 3 ปีที่แล้ว

    "...this will be on youtube for a million years so I might as well make it pretty..." I love you Sean Carroll.

  • @GEAsolar
    @GEAsolar 3 ปีที่แล้ว +14

    I realized that this serie of lectures will end eventually.
    We need more bigger ideas.

    • @papsaebus8606
      @papsaebus8606 3 ปีที่แล้ว

      Asolar I hope he begins new video series after biggest ideas is done.

    • @stephenbryant7873
      @stephenbryant7873 3 ปีที่แล้ว +1

      I think I could watch them again and learn more the second time around.

    • @Animuldok
      @Animuldok 3 ปีที่แล้ว

      Its physics, it will probably asymptote rather than reach a limit :D

  • @user-sb3wh3dd4v
    @user-sb3wh3dd4v 3 ปีที่แล้ว

    Dear Sean,
    You are a GREAT communicator. Over the last few years, and throughout this series. I have learned SO MUCH from you. Things that I have been curious about for over forty years, you explain so clearly.
    If I were a president or king, I would appoint you as one of the important communicators of important subjects.
    How much better would this world be if only we had more real scientists, engineers, doctors, nad other well educated ETHICAL people in government?
    The answer is simple. The world would be a MUCH better place.
    Thank you for all you do!

  • @ericgartner5201
    @ericgartner5201 ปีที่แล้ว

    I follow those lectures for a good number of month.very intrinsic and highly informative.mr.carroll does a wonderful work to communicate sientific and difficult content to the public.thank you very much indeed.

  • @renaudkener4082
    @renaudkener4082 3 ปีที่แล้ว +7

    I believe this serie of videos will reach the same status as "The Feynman Lectures on Physics" for the next generation of undergraduate students. Lucky guys :-)

  • @jonnysee2948
    @jonnysee2948 3 ปีที่แล้ว +1

    You’re so awesome Sean!!! Love you buddy!!! 💪🏽👍🏽❤️

  • @gilbertanderson3456
    @gilbertanderson3456 3 ปีที่แล้ว +3

    I'm loving your relaxed presentation in this series. You've inspired a great many people; I'm sure wikipedia's servers have felt the burden. I've spent many hours in follow-up reading after GIitU videos, and since we, your viewership, matter, and this IS the matter GIitU: here are my questions.
    WOW, not only are Bosons bosons, but Fermions can be bosons too ! Cooper pairs of electrons are bosons. (What force do they mediate?) Mesons (composed of a quark and an antiquark, two Fermions) are also bosons. Pions mediate the transformation (decay) of quarks. Tritium and ⁴He are bosons. Who knew all these Fermion collectives could be bosons?
    1) Why is hydrogen not a boson? Obviously it isn't or our sun would be a lot colder. 😡 But it is two spin ½ particles. ½+½≠1?
    This Wikipedia diagram en.m.wikipedia.org/wiki/File:Standard_Model_Of_Particle_Physics--Most_Complete_Diagram.png
    of the spin-0, spin-½ and spin-1 sectors before and after the spontaneous symmetry breaking of the Higgs condensation is quite fascinating. Is there REALLY an EM field, or is the overlap of (the crippled remaining half of) the weak hypercharge field and (the remaining crippled T³ component of) the weak isospin field what is reality. In describing the EM field are we in effect talking about the sun revolving around the earth (because obviously that is what we experience) ?
    2) Would a super-advanced alien laugh at Maxwell's equations and rewrite them in terms of the underlying fields?
    (And what about strong hypercharge and strong isospin? And if isospin has nothing to do with spin, WHAT IS IT? You sometimes get a little casual in your wording ( the "electron field" ). Are the muon and tau separate fields, or is there a single lepton field with the muon and tau as extreme excitations ?
    (Recent muon results seem to call into question lepton universality.) Can you point us to a list of all the underlying fields of the SM? Come on Sean, give us ALL THE GOOD STUFF ! )

  • @ericsvilpis1635
    @ericsvilpis1635 3 ปีที่แล้ว +3

    Sean, these videos have been absolutely amazing. Exactly what I’ve wanted to know about the way these things work! Thanks so much!

  • @colbynye5995
    @colbynye5995 3 ปีที่แล้ว +3

    Sooo sad to hear we are nearing the end! But thank you so much for doing these videos!

  • @menecross
    @menecross 3 ปีที่แล้ว +1

    I finaly understand the property Spin. Thank you!

  • @NalitaQubit
    @NalitaQubit 24 วันที่ผ่านมา

    You amaze me, Dr. Carroll.

  • @piyushf80
    @piyushf80 3 ปีที่แล้ว +1

    7:09 Prof.Carroll; hope this helps - "Sat"-"Yen"-"Dre"-"Nath" (Sat as in Sat, Yen as in Yen, Dre as in Dr.Dre, Nath as in Nathaniel)

  • @iczemi
    @iczemi 3 ปีที่แล้ว

    Thank you your lectures (vlogs) are simply fascinating.

  • @esperancaemisterio
    @esperancaemisterio 3 ปีที่แล้ว +5

    New video! Stopping everything and watching!

  • @TheMemesofDestruction
    @TheMemesofDestruction 2 ปีที่แล้ว

    33:00 - Thank you Professor!!

  • @JohnDlugosz
    @JohnDlugosz 3 ปีที่แล้ว +1

    Sean, you touched on complex dimensions in the episode on topology, and hinted at the fact that two complex dimensions is not quite the same as three real dimensions. But, you didn't come full circle (so to speak) when you got to spinnor fields.
    Also, after explaining that angle is defined via inner product in Hilbert space, you can _show_ how rotating 360 degrees leaves the vector different from what you started with, mathematically.

  • @qclod
    @qclod 3 ปีที่แล้ว +3

    These videos matter a lot to me!

  • @margaritahernandez7459
    @margaritahernandez7459 3 ปีที่แล้ว +3

    I love his lectures. Physics has always amazed me.

  • @rohitpandey3151
    @rohitpandey3151 3 ปีที่แล้ว +1

    I kind of like having my own space. So definitely more of a Fermion.

  • @wlegna18
    @wlegna18 3 ปีที่แล้ว +1

    Thanks for the video! I just bought your book and I look forward to reading it.

  • @alexandeur
    @alexandeur 3 ปีที่แล้ว +1

    Amazing! Thank you so much, Sean!

  • @venustus100
    @venustus100 3 ปีที่แล้ว +1

    Thank you!!

  • @LuciFeric137
    @LuciFeric137 ปีที่แล้ว

    Thank you professor Carroll.

  • @ThalesF75
    @ThalesF75 3 ปีที่แล้ว +8

    "of course it's the quantum state; what else could it be?"

  • @MadScienceWorkshoppe
    @MadScienceWorkshoppe 2 ปีที่แล้ว

    I'm going through some health things right now and the drugs give me weird and intense dreams. When I listen to these lectures at night somehow that fades away and I have mathy dreams instead, sleep longer, and don't wake up as often.

  • @jaschoudhury18
    @jaschoudhury18 3 ปีที่แล้ว

    "Why aren't atoms squishy?"...ahhh...that exam question we all dread!!

  • @Hulksterx
    @Hulksterx 3 ปีที่แล้ว +24

    Ahhh matter, something I can get a grip of.

    • @mezza205
      @mezza205 3 ปีที่แล้ว +2

      but can you ?

    • @oliverwinters1406
      @oliverwinters1406 3 ปีที่แล้ว

      Very good

    • @luckabuse
      @luckabuse 3 ปีที่แล้ว

      ideas can be matterial

    • @davemojarra2666
      @davemojarra2666 3 ปีที่แล้ว +1

      But not grammar, apparently.

    • @ctixbwi
      @ctixbwi 3 ปีที่แล้ว

      I can’t grasp everything equally well. What elementary particles contribute to that soap is slippery?!

  • @Cooldrums777
    @Cooldrums777 3 ปีที่แล้ว

    Very satisfying explanations of spin and wave function interchange. I have to admit that coffee cup example of 720 rotation was extremely satisfying. I definitely would not have grasped the concept without that example. Of course we are still missing an explanation as to exactly what object or abstract quantity the quantum wave function is rotating 720 degrees in relation to ( I presume it's not a Planck length version of Sean) but I accept your assertion that it's just too complicated to discuss here. The ribbon was excellent as well, and once you demonstrated the interchange and rotation it made sense immediately. This was an excellent lecture overall. A nice selection of big ideas were covered. Thank you Professor.

  • @youtou252
    @youtou252 3 ปีที่แล้ว

    Absolutely brilliant

  • @fsmvda
    @fsmvda 3 ปีที่แล้ว +1

    I hope we get to hear more about how the number of dimensions of spacetime affects the interchange operator. I can see how it would affect rotational symmetries and therefore angular momentum but I don't see how that argument about interchange causing us to have exactly two options could be modified.

    • @felipereyes8922
      @felipereyes8922 3 ปีที่แล้ว

      In one dimension, that is a row of particles constrained to move in this same row, the particles can't go around each other, so you can't actually tell if the particles are bouncing off each other or going through. In this case bosons and fermions are in some sense equivalent, and there are techniques to map systems of one dimensional fermions into bosons.

  • @nostradamuscat1131
    @nostradamuscat1131 3 ปีที่แล้ว +6

    your the F**king man Sean!!! the man! I love you

  • @bikashthapa7316
    @bikashthapa7316 3 ปีที่แล้ว +1

    thank you so much

  • @tizza963
    @tizza963 3 ปีที่แล้ว

    Amazing thank you so much

  • @Steve-xh3by
    @Steve-xh3by 3 ปีที่แล้ว

    First, thank you for doing these videos, Sean. Your ability to clearly explain complex ideas so that they are understandable to those of us who are not career physicists is truly unparalleled. That being said, my brain is hung up on the fundamental relationship between matter and “space.” Why do physicists refer to space as if it were a container or substrate that matter is “in” as opposed to just an emergent property of the matter itself? In other words, why don’t we just think that the structure of matter IS space rather than space existing as something independent from matter?

  • @robertzimmermann8315
    @robertzimmermann8315 ปีที่แล้ว

    Very good video! One (minor) correction to the Stern-Gerlach experiment: no-one has performed it yet with electrons as the Lorentz-force is too strong.

  • @rickharold7884
    @rickharold7884 3 ปีที่แล้ว

    awesome. So cool. Thx !

  • @annwwar
    @annwwar 3 ปีที่แล้ว +3

    Thank you for most interesting spin explanation I ever heard. I read before that matter is solid because of the EM repulsion forces between electrons. How does that fit in or compare to the Pauli pressure as the cause?

  • @jeannieh3661
    @jeannieh3661 3 ปีที่แล้ว

    Today I learned the difference between "squashy" and "squishy".👍👍💙💯🔥

  • @Bradgilliswhammyman
    @Bradgilliswhammyman ปีที่แล้ว

    been a fan of Sean's for a long long time. He did a great interview with Joe Rogan years ago that was fascinating and I hope connected with a audience that doesn't typically listen to someone like Sean Carrol.

    • @NFLbeatster
      @NFLbeatster ปีที่แล้ว

      He's done a few w Rogan. Which one is best?

  • @viewer3091
    @viewer3091 3 ปีที่แล้ว

    Thanks Sean.

  • @jankareaustinat310
    @jankareaustinat310 3 ปีที่แล้ว

    thank u carrol for beeing so consistent with us,this series will be like a sterter for a lot of peeps later on..thanks to corona too i guess

  • @Petrov3434
    @Petrov3434 3 ปีที่แล้ว +1

    One more question -- to which book do you refer when you say "it is in my book"?
    I have all your books (as well as from biologist Sean Carroll ;-)) ) -- in Audible format -- only two of your books have illustrations in PDF formats (Higgs and Big Picture)

  • @henryD9363
    @henryD9363 3 ปีที่แล้ว +1

    Planks constant is used as a measure of spin, as you have described. Planck's constant has units of angular momentum. If you fire a beam of up spin electrons at a target will that target gain classical angular momentum? (It might be too small to measure experimentally, but...)

  • @johnp1
    @johnp1 3 ปีที่แล้ว

    Thanks again for another great lecture. I'm wondering if we can use the field theories to explain how mater bends space-time, or the "bending" is just an approximation for graviton.

  • @robertshirley2645
    @robertshirley2645 3 ปีที่แล้ว +4

    I need one of those schrodinger’s cup so bad :))

  • @marcsmerlin
    @marcsmerlin 3 ปีที่แล้ว +9

    I have a question having to do with the Fermi pressure, specifically with the degeneracy pressure that keeps white dwarfs (or neutron stars) from collapsing any further. It would seem that the Pauli exclusion principle would, in some sense, be absolute: there's no forcing electrons (or neutrons) into the same quantum state. I assume that quantum mechanics doesn't break down, but somehow the Pauli exclusion barrier is circumvented for stars above a certain mass in both cases. How does gravity overcome this restriction?

    • @trucid2
      @trucid2 3 ปีที่แล้ว +5

      One way to get around the exclusion principle is to get rid of the particles. For example, if a star is supported by electron degeneracy pressure, at high enough pressure you would merge electrons with protons to create neutrons.

    • @Bill..N
      @Bill..N 3 ปีที่แล้ว +1

      @@trucid2 Indeed friend..A temporary respite for physics... Add enough additional matter to the neutron star tho, and ALL our descriptive abilities DO fail us..

    • @Bill..N
      @Bill..N 3 ปีที่แล้ว +2

      @@trucid2 Which brings up a simple concern.. GR tells us that the singularity produced by an efficient collapse of just a 10 solar mass object results in an INFINITE gravity field..The event horizon would be about 30 kilometers, AND surrounding a very mysterious "Object" of perhaps 200 mm that somehow exits outside our spacetime while LEAVING its infinite field behind..Does this expose a defect in our understanding of matmatiical descriptions, ot the theory, OR even our inability to understand reality itself? Inquiring minds would like to know...Peace.

    • @dankuchar6821
      @dankuchar6821 3 ปีที่แล้ว

      @@Bill..NYes, General Relativity predicts infinite density. Physicist don't like infinities. We assume it means there is something incomplete about general relativity.

    • @Bill..N
      @Bill..N 3 ปีที่แล้ว

      @@dankuchar6821 And yet GR has passed EVERY challenge to its legitimacy.. It doesn't play well with QM, (Mans greatest theory) which has its OWN renormalization issues..but both theories function incredibly well.. Peace friend..

  • @rsablosky
    @rsablosky 3 ปีที่แล้ว +1

    You talked about the Stern-Gerlach experiment, where instead being deflected through a range of angles, half of the silver atoms went one way, and half the other way. So, spin is quantized. But why???
    Intuitively, I accept that electrons are constrained to discrete orbits because only a whole number of standing waves can persist within a fixed boundary. Is there an analogous consideration for spin?
    One website told me, “Half-integer spins are consequence of group theory.… The spin operators and associated Hilbert space of spin states are governed by Lie SO(3) algebra, with resultant eigenvalues of ±½.” But I object to the word “consequence” here. Properties of the real world can’t be a *consequence* of group theory; it’s the other way round! (Isn't it?) Can you explain in English why spin is quantized?

  • @tookie36
    @tookie36 3 ปีที่แล้ว

    Thank geometry for Sean!

  • @Petrov3434
    @Petrov3434 3 ปีที่แล้ว +4

    An amazing lecture. Once again -- Sean Carroll's lecture made our day !!
    A question: In book reviews of Roger Penrose's "The Road to Reality" several reviewers, who apparently understand more than I, made surprising comments which I don't understand -- a la Penrose delivers the knock-out punch:
    --- Conservation of energy/momentum/angular momentum in General Relativity is non-local !!!
    What such comments really mean? What is their significance? Many thanks

    • @projectmalus
      @projectmalus 3 ปีที่แล้ว

      My guess is the effect from the field moves away to another "level" where it can play a part in the formation of another field.

  • @TheyCallMeNewb
    @TheyCallMeNewb 3 ปีที่แล้ว

    A visual demonstration.. And then a second? This proved a different peregrination today!

  • @swoop8047
    @swoop8047 3 ปีที่แล้ว

    28:22 that bit of Jamaican Patois had me giggling ^_^ thank you for the teachings!

  • @elck3
    @elck3 3 ปีที่แล้ว

    @Dr. Carroll, inside a black hole, right at the boundary that is infinitesimally close to the actual singularity, does matter take up any space?

  • @barefootalien
    @barefootalien 3 ปีที่แล้ว

    So a question for the Q&A if it's not too late... in the Stern-Gerlach experiment you drew the possible quantized values for measurements of particles for particles of spin-0 having 1 possible result; spin-1/2 having 2 possible results, and spin-1 having 3 possible results. But how does that pattern continue? Would a Gravitino with spin 3/2 have 4 results, and a Graviton with spin 2 have 5? Or does it just alternate back and forth with the results getting further and further apart, so a Gravitino would have 2 results at 3/2 and -3/2 while a Graviton would have 3 at 2, 0, and -2? Could this point to any insights we might get about the graviton through other kinds of tests, despite not having detected them?

  • @tonydarcy1606
    @tonydarcy1606 3 ปีที่แล้ว +3

    The only spins I understand are 33, 45 and 78. But they do involve Pi !

    • @tomasnemec5680
      @tomasnemec5680 3 ปีที่แล้ว

      Not many people out there still get this I am afraid ...

    • @zebrawien
      @zebrawien 3 ปีที่แล้ว

      ​@@tomasnemec5680 Based on your data of the universe? - I guess. Why not break the ice and have the people participate? :)
      Simplified: 33, 45 and 78 is the number of spins per minute of standard vinyl records. The record is a circle. Pi is the ratio of the circumference of a circle to its diameter. :)

  • @stevebrown661
    @stevebrown661 3 ปีที่แล้ว

    Hi Sean thanks for this riveting series of vids. You mentioned spin zero gravitons(which may not exist) , or more generally spin zero particles in a scalar field - exhibiting a 'breathing mode'. How does this square up with invariance under rotation of a scalar field please, Sean?
    (Does Higgs exhibit a breathing mode?)

  • @ags5377
    @ags5377 3 ปีที่แล้ว

    One small correction: the example of the electron going through the Stern-Gerlach experiment is not correct. As it is a charged particle is it subjected to the Lorentz force which will distort the clear separation in 2 discrete states. The experiment is usually done with charge neutral particles such as silver atoms.

  • @alachance2010
    @alachance2010 3 ปีที่แล้ว

    25:00
    Fermions are described by spinor field, while bosons by tensor field

  • @crontemisto8994
    @crontemisto8994 3 ปีที่แล้ว

    Does the Pauli Exclusion Principle relate to a particular force that keeps particles away from each other? I.E., what happens physically, say in a neutron star, to keep particles from occupying the same location?

  • @haydarmasud635
    @haydarmasud635 3 ปีที่แล้ว

    Hello Dr, Carroll, thank you for breaking down such big ideas into the simplest form that even the dumbest people like me can understand. I hope you will make a lecture on tensor calculus and how to manipulate indices since it is at the heart of Relativity.

  • @callycraig3132
    @callycraig3132 3 ปีที่แล้ว +1

    If and when is this series going to come out on a set of dvds?

  • @sebastiandierks7919
    @sebastiandierks7919 3 ปีที่แล้ว

    At 24:07 you mention that "whether bosons and fermions are the only possibilities depends on the dimension of spacetime". Could you elaborate? I'm a physics master's student and in my QM II lecture we basically exactly followed your line of argument (of course more mathy and more detailed but still). So it's not clear to me how the argument that the square of the interchange operator is 1, i.e. having eigenvalues of 1 and -1 such that psi(X2,X1)=+ or - psi(X1,X2) but excluding the possibility of arbitrary e^(i*theta) phases, depends on the dimension of space.

  • @valrossen
    @valrossen 3 ปีที่แล้ว

    What is the cause and what is the effect in the Pauli Exclusion Principle? Is the spin causing the minus-sign? Or is the minus-sign causing the spin? Or do the different underlying behavior of the fields cause both? Or are they all independently just different things that happen to correlate?

  • @BT-kf4kx
    @BT-kf4kx 3 ปีที่แล้ว

    Hi Dr. Carroll, can you plesae do a video explaining about the myth of "warp speed" that we keep seeing in movie such as star trek and such? I am very curious what's the correlation between gravity and electrons?

  • @bretnetherton9273
    @bretnetherton9273 3 ปีที่แล้ว

    Awareness is known by awareness alone.

  • @EarlWallaceNYC
    @EarlWallaceNYC 3 ปีที่แล้ว

    So from where comes the exclusion pressure. The Exclusion Principle seems binary: How does it say anything about particles which are "close" to the same state?
    Another insightful lecture/video. Thanks.

  • @tr48092
    @tr48092 3 ปีที่แล้ว +1

    You gave an amazing visual analogy for spin 1/2 particles with a coffee cup in your hand that has to be spun twice around to get back to the original state. Is there such an analogy for spin 3/2 or 5/2 particles and, if not, does that lack of a visual analogy say anything about the real possibility of such particles existing?

    • @JohnDlugosz
      @JohnDlugosz 3 ปีที่แล้ว

      odd multiples of spin 1/2 all behave the same way.
      Composite particles and systems of particles can have spin 3/2 etc, and orbitals can contain higher spin multiples. At low energy, so you can't resolve the components, it behaves the same as a fundamental particle would.
      Theorized supersymmetric particles include spin 3/2 gravitino as he mentioned in the video.

  • @Toocrash
    @Toocrash 3 ปีที่แล้ว

    Vectors don't change under Bro°😅 - tis information is applicable to so much, it's distracting. Sean thank you!

  • @Chirality452
    @Chirality452 3 ปีที่แล้ว

    One this issue of spin in a fermion such as the electron. The electron is a quantum field not a literal point particle. A classical field can have an angular momentum so does the quantum field have an angular momentum in a similar sense? That was what I understood from your comments about the paper you published with a student.

  • @davidhand9721
    @davidhand9721 3 ปีที่แล้ว

    Is there an actual energy gradient to Fermi pressure?

  • @baogiangsongque5507
    @baogiangsongque5507 3 ปีที่แล้ว

    Thank you Professor Carroll, Sean for the excellent lecture. how ever, keep in your mind that 10% is a part of true and the rest 90% is just a story. we are waitting for your next part of true physical lecture.
    8:00 why one atom can not stack on top another one.
    1. Because the atom want like that = thinking = a story =?
    2. Because the matter have 2 forms: order energy mechanic and none order energy mechanic. After big bang all form of none order energy mechanic (FONOEM) transform into the particles. then all all form of order energy mechanic transform into the atom.
    3. Matter have 2 mains state mechanic: state of lower order energy mechanic order energy mechanic and state of higher standard energy local reference mechanic. all atoms are usually standard energy local reference mechanic which called earth or solar space mechanic.
    Imagine if an atom outside of milky way or solar system enter into solar space. due on this atom motion creating a different energy vector and so on. We call anti-matter or none unique reference energy frame.
    Here the experiment: on the car running at constant speed as the car energy reference frame is the same. You must use force or energy to used the knife to cut the apple base on they are in the standard order energy mechanic and the same order energy mechanic. If the knife is being in the car running and the apple is being outside of the car. You can cut easy or can not cut the apple at all base on they are same form but in different state of vector energy.
    These explain clearly how chemical reaction and so on by physical term. May be no more rocket era enter into the space.

  • @StumpyMason_
    @StumpyMason_ 3 ปีที่แล้ว +1

    I think i'm starting to get it.. When do I get my phd?

  • @4pharaoh
    @4pharaoh 3 ปีที่แล้ว

    Humm? How is the experiment done that allows you to "rotate" a fermion 360 or 720?

  • @NuclearIsShit
    @NuclearIsShit 3 ปีที่แล้ว

    We can't squish a table, but does the table eventually degrade or lose its energy or charge over time if it's protected by environmental factors?

  • @sagmilling
    @sagmilling 3 ปีที่แล้ว +1

    New video! Popcorn time.
    Question, valence electrons must be separate "shapes" to have different psi, but the quantity of valence states increases with atomic number. What is actually changing?

    • @felipereyes8922
      @felipereyes8922 3 ปีที่แล้ว +1

      The tl;dr summary is that pauli exclusion is still followed because even though you have more electrons in the same valence energy level, there are more distinct quantum states that yield this result. In more detail, higher atomic numbers have more electrons. These start filling up the available energy states, beginning with the lowest, innermost states. Each new energy level is like a shell around the nucleus. Valence electrons sit in the outermost shell, and since they have the highest energy, they are the ones that bond with other atoms. The thing is, each shell can hold a different number of electrons. Although they share the same energy, the electrons have other properties that are different and so they can sit in the same shell without violating Pauli exclusion. The actual property is angular momentum, as you increase the energy there are more distinct angular momentum states that yield the same result.

  • @wdacademia2329
    @wdacademia2329 3 ปีที่แล้ว

    To what extent is the non-squishyness attributed to Fermi-pressure rather than the electromagnetic force? I imagine that if the electromagnetic force was weaker, then Fermi-pressure would also be weaker. The "electron-wavefunction" around a nucleus would be larger and thus two atoms could overlap more before Fermi pressure really kicks in. Is that right?

  • @kx4532
    @kx4532 3 หลายเดือนก่อน

    I don't know about 1% but you can squeeze piezoelectric crystals to create a voltages and apply voltage to deform the piezoelectric crystals.

  • @Cooldrums777
    @Cooldrums777 3 ปีที่แล้ว

    Is a monochromatic and coherent LASER beam composed of Bosons that are all in the same quantum state?

  • @sebastiandierks7919
    @sebastiandierks7919 3 ปีที่แล้ว

    At 40:26 you say that "spin-1 really means spin of 1 hbar". I've heard this so often online and even in lectures and I'm still confused about this. A particle in the state |s,m> satisfies the eigenvalue equations
    S^2 |s,m> = s(s+1) hbar^2 |s,m>
    S_z |s,m> = m hbar |s,m>
    where S is spin operator (I'm not able to draw the vector arrow on top) and S_z is its z-component. s takes values of 0, 1/2, 1,... and for given s, m takes values from s, s-1,...-s+1,-s.
    That said, taking the first eigenvalue equation, shouldn't the absolute value of the spin vector of a spin-1 particle be the square root of the eigenvalue of the operator S^2? That would be square root of 1*(1+1) hbar^2 = sqrt(2)*hbar. Not 1*hbar. Similarly, the spin of a spin-1/2 particle would be sqrt(1/2*3/2) hbar=sqrt(3)/2*hbar.
    Of course, the second eigenvalue equation shows that a spin-1 particle can have a z-component of its spin vector of 1, 0 or -1 hbar. Or a spin-1/2 particle with spin up would have a z-component of hbar/2. But I think at this moment in the video you're talking about the absolute value of the spin, not the z-component.

  • @joshhickman77
    @joshhickman77 3 ปีที่แล้ว

    So, I'm imagining gravity as a vector field, and it doesn't seem like it would have spin-2, because up and down are different. Is the spin-2 from the idea that, in 4-d spacetime you'd swap up/down and future/past? I mean, it seems gravity is symmetric that way. [I'm thinking and reversing all components of the vector _including time_ is the thing, yes? pi radians in all dimensions?]

  • @barryzeeberg3672
    @barryzeeberg3672 หลายเดือนก่อน

    I am trying to get a more intuitive understanding of the quantum fields.
    (1) Say that, in the normal world, we had a macroscopic object like e.g. a finger. Would there be an arrangement of vibrations in the quantum field that looks like a finger, or would the finger be represented by something like a Fourier Transform?
    (2) Say that in the real world my finger pushes a small ball. What is the representation of that in the quantum field? Can I actually make something happen in the quantum field by something that I do in the real world? I would think that you need some special device (like a laser, etc, not just my finger) to manipulate a vibration in the quantum field?

  • @briancannard7335
    @briancannard7335 3 ปีที่แล้ว

    Thank you for the 360 degrees user friendliness. It adds a lot of charm to your way of explaining. I wish you to not talk and write at the same time more often. I'm curious how do you manage to keep your eyebrows calm when that happens? Have you trained to keep friendly facial expression so your student keep listening? :-) One of the greatest teachers in the world! For sure. Thank you for your Mission!